cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð³Ð¾ÑÑÑÐµÐ¹ ÐºÐ¾Ð²ÐºÐ¸ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²Ð¾Ðº Ð¼ÐµÐ´Ð½ÑÑ Ð³Ð¸Ð»ÑÐ· ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¸Ð·Ð°ÑÐ¾ÑÐ°
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÑÐ´ÑÐ¼ÐµÑ, ÐÐ»ÐµÐºÑÐµÐ¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: Ð¨ÑÐ°Ð¼Ð¿Ð¾Ð²ÐºÐ° Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð² Ð³Ð¾ÑÑÑÐ°Ñ
ÐÐ°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸
ÐÑÐ»Ð¸Ð²ÐºÐ¸ Ð¼ÐµÐ´Ð½ÑÐµ
ÐÐµÑÐ°Ð»Ð¸ Ð¼Ð°ÑÐ¸Ð½ Ð»Ð¸ÑÑÐµ

description: Ð Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¸ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ñ Ð¸Ð·Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸Ñ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÐ¸Ð»ÑÐ·Ð° ÐºÑÐ¸ÑÑÐ°Ð»Ð»Ð¸Ð·Ð°ÑÐ¾ÑÐ°Â» Ð¼ÐµÑÐ¾Ð´Ð¾Ð¼ Ð¿ÑÐ¾ÑÑÐ¶ÐºÐ¸ Ð½Ð° Ð¾Ð¿ÑÐ°Ð²ÐºÐµ, Ð±ÑÐ»Ð¾ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ ÐºÐ¾Ð½ÐµÑÐ½Ð¾-ÑÐ»ÐµÐ¼ÐµÐ½ÑÐ½Ð¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ Ð³Ð¸Ð±ÐºÐ¸ Ð² Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð½Ð¾Ð¼ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐµ Simufact.Forming. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð° ÑÐ°ÐºÐ¶Ðµ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐ°ÑÑÐµÑÐ¾Ð² Ð±ÑÐ»Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð¿Ð¾Ð·Ð²Ð¾Ð»Ð¸Ð»Ð¸ Ð¿Ð¾Ð´Ð¾Ð±ÑÐ°ÑÑ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÑÑÐµÐµ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð¾ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ° Ñ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸ÐµÐ¼ Ð³Ð¾Ð´Ð¾Ð²Ð¾Ð³Ð¾ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÑÑÐµÐºÑÐ°. ÐÐ°Ð½Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð²Ð¾Ð¿ÑÐ¾ÑÐ°Ð¼ ÑÐµÑÐ½Ð¸ÐºÐ¸ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¸ ÑÐ°Ð±Ð¾ÑÐµ Ñ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð² ÑÐµÑÐµ, Ð¾ÑÐ²ÐµÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾Ð¹ ÑÐ°Ð½Ð¸ÑÐ°ÑÐ¸Ð¸ Ð¸ Ð¿Ð¾Ð¶Ð°ÑÐ½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð° ÑÐ°Ð±Ð¾ÑÐµÐ¼ Ð¼ÐµÑÑÐµ.
The relative efficiency of clinical and actuarial methods in the prediction of University freshman success.
Creators: name: Simmons, Helen
Publisher: name: University of British Columbia
Year: 2012

description: The purpose of this study was to investigate the relative, efficiency of clinical and actuarial methods in predicting success of University freshmen. The clinical predictions were based on the judgements of two University counselors. The information available to the counselors consisted of an interview report sheet, scores from tests intended to measure general learning ability, English placement, mathematical ability, and an expression of vocational interests, as well as identifying information such as name, age, and other similar kinds of data. The actuarial prediction was based on a regression equation built on scores of two tests, one of mathematical ability, and one of English placement. These scores were among those available to the counselors. The regression equation was cross-validated in the study, since it was originally built on the scores obtained on these two tests by a previous sample of University freshmen, chosen on the same set of criteria. Predictions were made for 158 Arts freshmen registered at the University of British Columbia for courses amounting to exactly 15 units of credit (including two laboratory sciences and an introductory mathematics course of freshmen level). Each case included in the sample, had availed himself of University counselling and each counselor predicted only for those students he had personally counselled. One counselor predicted for 78 subjects, and, the other for 80 subjects. Predictions to success were made in terms of a "pass-fail” dichotomy. The relative efficiency of the two methods was tested against four criteria: better than chance prediction, homogeniety, relatedness, and "hit" predictions. In testing for "better-than-chance" prediction the accuracy of each method was compared with "chance prediction" accuracy, where "chance" accuracy was considered to be 50 per cent. In testing for homogeniety, the number of cases assigned to either category of the success dichotomy by each method was compared. In testing relatedness of predictions, a comparison was made in terms of agreement by the two methods in assigning, a given subject to one or the other category of the dichotomy. Finally, in comparing "hit" predictions, the number of predictions which were in fact correct predictions made by each method were used as the basis for comparison. Analysis of the obtained results showed no significant difference in efficiency of the actuarial and clinical methods in predicting success of University freshmen. Both methods were shown to be significantly better than chance predictors.
MPEC 2023-K107 : 2023 KT1
Creators: name: Minor Planet Center Staff
Publisher: name: The Minor Planet Center
Year: 2023
Subjects: subject: Small Solar System bodies
valueUri: http://astrothesaurus.org/uat/1469
subject: 2023 KT1

description: The Minor Planet Electronic Circulars contain information on unusual minor planets, routine data on comets and natural satellites, and occasional editorial announcements.  They are published on behalf of Division F of the International Astronomical Union by the Minor Planet Center, Smithsonian Astrophysical Observatory, Cambridge, MA 02138, U.S.A.
title: Ð¡Ð±Ð¾ÑÐ½Ð¸Ðº Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÑ Ð´Ð°Ð½Ð½ÑÑ Ð¿Ð¾ Ñ Ð¸Ð¼Ð¸Ð¸ Ð¸ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸Ð¸ Ð´Ð»Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¸ ÑÐ°ÑÑÐ¸ÑÐµÐ½Ð¸Ñ Ð¸Ñ ÐºÑÑÐ³Ð¾Ð·Ð¾ÑÐ°
Creators: name: ÐÐ»Ð¸Ð½Ð¾Ð², ÐÐµÐ²
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2019
Subjects: Ð¥Ð¸Ð¼Ð¸Ñ
Ð­ÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ

description: Ð ÑÐ±Ð¾ÑÐ½Ð¸ÐºÐµ ÑÐ¾Ð±ÑÐ°Ð½Ñ Ð²ÑÑÐºÐ°Ð·ÑÐ²Ð°Ð½Ð¸Ñ Ð¸ Ð¼ÑÑÐ»Ð¸ ÑÑÐµÐ½ÑÑ-ÑÐ¸Ð¼Ð¸ÐºÐ¾Ð² Ð¸ ÑÐºÐ¾Ð»Ð¾Ð³Ð¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð¸ÑÐµÐ»ÐµÐ¹ Ð´ÑÑÐ³Ð¸Ñ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¹ Ð¸ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐµÐ¹, Ð¿ÐµÐ´Ð°Ð³Ð¾Ð³Ð¾Ð², Ð¾ÑÑÑÐ²ÐºÐ¸ Ð¸Ð· Ð¾ÑÐ²ÐµÑÐ¾Ð² ÑÑÐ°ÑÐ¸ÑÑÑ.
ÐÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ Ð² ÑÐºÐ¾Ð»Ðµ Ð¸ Ð² Ð²ÑÐ·Ðµ Ð¼Ñ ÑÐ°ÑÐµ Ð²ÑÐµÐ³Ð¾ ÑÑÐ°Ð»ÐºÐ¸Ð²Ð°ÐµÐ¼ÑÑ Ñ ÑÐ¸Ð¼Ð¸ÐµÐ¹
Ð¸ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÐµÐ¹ ÐºÐ°Ðº Ñ ÐµÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð½Ð°ÑÑÐ½ÑÐ¼Ð¸ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ð°Ð¼Ð¸. ÐÐ¾ Ð² Ð½Ð¸Ñ ÐµÑÑÑ Ð¸ Ð´ÑÑÐ³Ð¸Ðµ
Ð³ÑÐ°Ð½Ð¸, Ð·Ð½Ð°Ð½Ð¸Ðµ ÐºÐ¾ÑÐ¾ÑÑÑ Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÐµÑ Ð½Ðµ ÑÐ¾Ð»ÑÐºÐ¾ Ð»ÑÑÑÐµ Ð¿Ð¾Ð½ÑÑÑ ÑÐ¸Ð¼Ð¸Ñ Ð¸ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ
ÐºÐ°Ðº ÑÑÐµÐ±Ð½ÑÐµ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ, Ð½Ð¾ Ð¸ Ð¾ÑÐµÐ½Ð¸ÑÑ Ð¸Ñ ÑÐ¾Ð»Ñ Ð¸ Ð·Ð½Ð°ÑÐµÐ½Ð¸Ðµ Ð² ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸
Ð½Ð°ÑÐµÐ³Ð¾ Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð·Ð·ÑÐµÐ½Ð¸Ñ, Ð¼Ð¸ÑÐ¾Ð²Ð¾Ð·Ð·ÑÐµÐ½Ð¸Ñ ÑÐµÐ»Ð¾Ð²ÐµÐºÐ° XXI Ð².
ÐÐ´Ð½Ð¸Ð¼ Ð¸Ð· Ð¿ÑÐ¸Ð¼ÐµÑÐ¾Ð² ÑÐ°ÐºÐ¸Ñ Ð³ÑÐ°Ð½ÐµÐ¹ ÑÐ²Ð»ÑÑÑÑÑ Ð¿ÐµÐ³Ð½Ð¸Ð¾ÑÐ¸Ð¼Ð¸Ñ Ð¸ Ð¿ÐµÐ³Ð½Ð¸Ð¾ÑÐºÐ¾Ð»Ð¾Ð³Ð¸Ñ,
Ð² ÐºÐ¾ÑÐ¾ÑÑÑ Ð² Ð²ÐµÑÐµÐ»Ð¾Ð¹ Ð¸ ÑÑÑÐ»Ð¸Ð²Ð¾Ð¹ ÑÐ¾ÑÐ¼Ðµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð½Ðµ ÑÐ¾Ð»ÑÐºÐ¾ Ð²Ð°Ð¶Ð½ÐµÐ¹ÑÐ¸Ðµ
Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¼Ð¸ÑÐ°, Ð½Ð¾ Ð¸ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð¶Ð¸Ð·Ð½Ð¸ Ð¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ°Ð¶Ð´Ð¾Ð³Ð¾ Ð¸Ð·
Ð½Ð°Ñ, Ð½Ð°ÑÐµÐ³Ð¾ Ð»Ð¸ÑÐ½Ð¾Ð³Ð¾ Ð¾ÑÐ½Ð¾ÑÐµÐ½Ð¸Ñ Ðº Ð¾ÐºÑÑÐ¶Ð°ÑÑÐµÐ¹ ÑÑÐµÐ´Ðµ, ÐµÐµ Ð·Ð°Ð³ÑÑÐ·Ð½ÐµÐ½Ð¸Ñ, Ð³ÑÑÐ´ÑÑÐ¸Ð¼ Ð¿Ð¾ÐºÐ¾Ð»ÐµÐ½Ð¸ÑÐ¼ Ð·ÐµÐ¼Ð»ÑÐ½.
Â«ÐÐµÑÐµÐ»ÑÐµÂ» Ð½Ð°ÑÐºÐ¸ (ÑÐ¾ÑÐ½ÐµÐµ Â«Ð²ÐµÑÐµÐ»ÑÐµÂ» ÑÐ°Ð·Ð´ÐµÐ»Ñ Ð½Ð°ÑÐº) Ð¿Ð¾Ð·Ð²Ð¾Ð»ÑÑÑ Ð·Ð°ÑÑÐ¾Ð½ÑÑÑ
Ñ Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð´Ð¾Ð¿Ð¾Ð»Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐµ Â«ÑÑÑÑÐ½Ñ ÑÐµÑÐ´ÑÐ° Ð¸ ÑÐ¼Ð°Â», ÑÐ¾ÑÐ¼Ð¸ÑÑÑÑ Ð¸ ÑÐºÑÐµÐ¿Ð»ÑÑÑ Ð¸Ñ Ð½ÑÐ°Ð²ÑÑÐ²ÐµÐ½Ð½ÑÐµ, ÐºÑÐ»ÑÑÑÑÐ½ÑÐµ Ð¸ Ð³ÑÐ¼Ð°Ð½Ð¸ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÑÑÐ¾Ð¸.
ÐÐ°ÑÐµÑÐ¸Ð°Ð» Ð½Ð°ÑÑÐ¾ÑÑÐµÐ³Ð¾ Ð¸Ð·Ð´Ð°Ð½Ð¸Ñ ÑÐ¿Ð¾ÑÐ¾Ð±ÐµÐ½ Ð¿Ð¾Ð²ÑÑÐ¸ÑÑ Ð¸Ð½ÑÐµÑÐµÑ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ðº ÑÐ¸Ð¼Ð¸Ð¸ Ð¸ ÑÐºÐ¾Ð»Ð¾Ð³Ð¸Ð¸, Ð² ÑÐ¾Ð¼ ÑÐ¸ÑÐ»Ðµ Ð¸ Ð·Ð° ÑÑÐµÑ Ð¸Ñ Ð»ÑÐ±Ð¾Ð·Ð½Ð°ÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸. Ð Ð»ÑÐ±Ð¾Ð·Ð½Ð°ÑÐµÐ»ÑÐ½Ð¾ÑÑÑ, ÐºÐ¾ Ð²ÑÐµÐ¼Ñ Ð¿ÑÐ¾ÑÐµÐ¼Ñ, ÐµÑÑÑ ÐºÐ»ÑÑ Ðº Ð·Ð½Ð°Ð½Ð¸ÑÐ¼ Ð¸ Ðº ÑÑÐ¿ÐµÑÑ. ÐÐ°Ð½Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÑÐ°Ð²Ð¸Ñ ÑÐ²Ð¾ÐµÐ¹ ÑÐµÐ»ÑÑ Ð¿ÑÐ¸Ð²Ð»ÐµÑÑ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ¸ÑÐ°ÑÐµÐ»Ñ Ð¸ Ðº ÑÐºÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¼ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ð°Ð¼.
Finite temperature spin-dynamics and phase transitions in spin-orbital models
Creators: name: Chen, C. -C.
name: Moritz, B.
name: Brink, J. van den
name: Devereaux, T. P.
name: Singh, R. R. P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: We study finite temperature properties of a generic spin-orbital model relevant to transition metal compounds, having coupled quantum Heisenberg-spin and Ising-orbital degrees of freedom. The model system undergoes a phase transition, consistent with that of a 2D Ising model, to an orbitally ordered state at a temperature set by short-range magnetic order. At low temperatures the orbital degrees of freedom freeze-out and the model maps on to a quantum Heisenberg model. The onset of orbital excitations causes a rapid scrambling of the spin spectral weight away from coherent spin-waves, which leads to a sharp increase in uniform magnetic susceptibility just below the phase transition, reminiscent of the observed behavior in the Fe-pnictide materials.
description: 4 pages
Merging Cold Fronts in the Galaxy Pair NGC 7619 and NGC 7626
Creators: name: Randall, S. W.
name: Jones, C.
name: Kraft, R.
name: Forman, W. R.
name: O'Sullivan, E.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We present results from {\it Chandra} observations of the galaxy pair NGC 7619 and NGC 7626, the two dominant members of the Pegasus group. The X-ray images show a brightness edge associated with each galaxy, which we identify as merger cold fronts. The edges are sharp, and the axes of symmetry of the edges are roughly anti-parallel, suggesting that these galaxies are falling towards one another in the plane of the sky. The detection of merger cold fronts implies a merging subgroup scenario, since the alternative is that the galaxies are falling into a pre-existing $\sim1$ keV halo without a dominant galaxy of its own, and such objects are not observed. We estimate the 3D velocities from the cold fronts and show that the velocity vectors are indeed most likely close to the plane of the sky, with a relative velocity of $\sim1190\kms$. The relative velocity is consistent with what is expected from the infall of two roughly equal mass subgroups whose total viral mass equals that of the Pegasus group. We conclude that the Pegasus cluster is currently forming from a major merger of two subgroups, dominated by NGC 7619 and NGC 7626. NGC 7626 contains a strong radio source, a core with two symmetric jets and radio lobes. Although we find no associated structure in the X-ray surface brightness map, the temperature map reveals a clump of cool gas just outside the southern lobe, presumably entrained by the lobe, and an extension of cooler gas into the lobe itself. The jet axis is parallel with the projected direction of motion of NGC 7626 (inferred from the symmetry axis of the merger cold front), and the southern leading jet is foreshortened as compared to the northern trailing one, possibly due to the additional ram pressure the forward jet encounters.
description: 11 pages, 9 figures. Accepted to ApJ. Minor changes to be consistent with accepted version
LED agricoltori nello spazio
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

Al posto di pesanti, ingombranti e poco ecologiche lampadine tradizionali, gli esperti credono che diodi ad emissione luminosa rossi e blu potranno essere la soluzione per la coltivazione di piante (tipo insalata e pomodori) nello spazio, magari durante missioni di lunga durata come quella su Marte
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÑÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¼ÑÐ¶ÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ²Ð¸, ÑÐµÐ°Ð»Ð¸Ð·ÑÐµÐ¼Ð¾Ð¹ Ð² ÑÐ¾Ð·Ð½Ð¸ÑÐ½ÑÑ ÑÐ¾ÑÐ³Ð¾Ð²ÑÑ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸ÑÑ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¢ÐºÐ°ÑÐµÐ½ÐºÐ¾, ÐÐ»Ð°Ð´Ð¸ÑÐ»Ð°Ð²
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð¾Ð±ÑÐ²Ð¸
ÐºÐ°ÑÐµÑÑÐ²Ð¾ Ð¾Ð±ÑÐ²Ð¸
ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ Ð¾Ð±ÑÐ²Ð¸
ÑÐ¾Ð²Ð°ÑÐ¾Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ðµ
ÑÐ¾Ð²Ð°ÑÐ¾ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð¸Ðµ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐºÐ¾Ð¶Ð°Ð½Ð°Ñ Ð¾Ð±ÑÐ²Ñ. Ð¦ÐµÐ»ÑÑ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÑÑÐºÐ¸Ñ ÑÐ²Ð¾Ð¹ÑÑÐ² Ð¸ Ð¾ÑÐµÐ½ÐºÐ° ÐºÐ°ÑÐµÑÑÐ²Ð° ÐºÐ¾Ð¶Ð°Ð½Ð¾Ð¹ Ð¾Ð±ÑÐ²Ð¸. ÐÐ° Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ð¸ Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ ÑÐµÐ»Ð¸ Ð±ÑÐ»Ð¸ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ñ, Ð¿ÑÐ¸Ð¼ÐµÐ½ÑÐµÐ¼ÑÐµ Ð´Ð»Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð° Ð¾Ð±ÑÐ²Ð¸, Ð¿ÑÐ¾ÑÐµÑÑ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð°, ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ Ð¸ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½Ñ, Ð¿Ð¾ÑÑÐµÐ±Ð¸ÑÐµÐ»ÑÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð¸ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¾ÑÐµÐ½ÐºÐ° ÐºÐ°ÑÐµÑÑÐ²Ð° ÐºÐ¾Ð¶Ð°Ð½Ð¾Ð¹ Ð¾Ð±ÑÐ²Ð¸. Ð ÐºÐ°ÑÐµÑÑÐ²Ðµ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð±ÑÐ» Ð²ÑÐ±ÑÐ°Ð½ Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½Ñ ÐºÐ¾Ð¶Ð°Ð½Ð¾Ð¹ Ð¾Ð±ÑÐ²Ð¸, ÑÐµÐ°Ð»Ð¸Ð·ÑÐµÐ¼Ð¾Ð¹ Ð² Ð¼Ð°Ð³Ð°Ð·Ð¸Ð½Ðµ Â«Ð­ÐºÐ¾Ð½Ð¸ÐºÐ°Â». ÐÑÐµÐ½ÐºÐ° ÐºÐ°ÑÐµÑÑÐ²Ð° Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»Ð°ÑÑ Ð¿Ð¾ Ð½ÐµÑÐºÐ¾Ð»ÑÐºÐ¸Ð¼ Ð±ÑÐµÐ½Ð´Ð°Ð¼, Ð²ÑÐ¿ÑÑÐºÐ°ÑÑÐ¸Ñ Ð½Ð° Ð¾Ð±ÑÐ²Ð½Ð¾Ð¹ ÑÑÐ½Ð¾Ðº Ð½Ð°Ð¸Ð±Ð¾Ð»ÐµÐµ Ð´ÐµÑÐµÐºÑÐ½ÑÑ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ñ. ÐÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ ÑÐ¾ÑÐ³Ð¾Ð²Ð»Ð¸, Ð¸Ð·ÑÑÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð³Ð¾ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²ÐµÐ½Ð½ÑÑ ÑÐ²ÑÐ·ÐµÐ¹ Ð¸ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ Ð¿Ð¾ Ð¿Ð¾ÑÑÐ°Ð²ÐºÐ°Ð¼ ÑÐ¾Ð²Ð°ÑÐ¾Ð². ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÐ¸ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð¾Ð±ÑÐ²Ð¸ Ð² ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¼ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸Ð»Ð¸ÑÑ Ð² Ð»Ð°Ð±Ð¾ÑÐ°ÑÐ¾ÑÐ½ÑÑ ÑÑÐ»Ð¾Ð²Ð¸ÑÑ. ÐÐ»Ñ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ñ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð¾Ð² Ð±ÑÐ»Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ñ Ð½Ð¾ÑÐ¼Ð°ÑÐ¸Ð²Ð½Ð°Ñ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ñ, ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð°Ñ Ð¸ ÑÑÐµÐ±Ð½Ð°Ñ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ° Ð¿Ð¾ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐµÐ¼Ðµ, Ð° ÑÐ°ÐºÐ¶Ðµ ÐÐ½ÑÐµÑÐ½ÐµÑ-ÑÐµÑÑÑÑÑ.
Nonequilibrium statistical mechanics of shear flow: invariant quantities and current relations
Creators: name: Baule, A.
name: Evans, R. M. L.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Statistical Mechanics (cond-mat.stat-mech)
subject: Soft Condensed Matter (cond-mat.soft)
subject: FOS: Physical sciences

description: In modeling nonequilibrium systems one usually starts with a definition of the microscopic dynamics, e.g., in terms of transition rates, and then derives the resulting macroscopic behavior. We address the inverse question for a class of steady state systems, namely complex fluids under continuous shear flow: how does an externally imposed shear current affect the microscopic dynamics of the fluid? The answer can be formulated in the form of invariant quantities, exact relations for the transition rates in the nonequilibrium steady state, as discussed in a recent letter [A. Baule and R. M. L. Evans, Phys. Rev. Lett. 101, 240601 (2008)]. Here, we present a more pedagogical account of the invariant quantities and the theory underlying them, known as the nonequilibrium counterpart to detailed balance (NCDB). Furthermore, we investigate the relationship between the transition rates and the shear current in the steady state. We show that a fluctuation relation of the Gallavotti-Cohen type holds for systems satisfying NCDB.
description: 24 pages, 11 figures
title: ÐÑÑÐ¸ÑÐ°ÐµÐ¼Ð¾ÑÑÑ Ð±ÐµÑÐ¾Ð½Ð½ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹ Ð¼Ð¾ÑÑÐºÐ¸Ñ Ð³Ð¸Ð´ÑÐ¾ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹ Ð¸ Ð¸Ñ ÑÐµÐ¼Ð¾Ð½Ñ
title: Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ°Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ñ
titleType: Subtitle
Creators: name: ÐÐ¾ÑÐ¾ÑÐºÐ¾Ð², ÐÐ¸ÐºÐ¸ÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐÐµÑÐ¾Ð½Ð½ÑÐµ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð³Ð¸Ð´ÑÐ¾ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ñ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ð¹
ÐÐ¾ÑÑÐºÐ¸Ðµ Ð»ÑÐ´Ñ
Ð¸ÑÑÐ¸ÑÐ°ÐµÐ¼Ð¾ÑÑÑ
Ð»ÐµÐ´Ð¾Ð²Ð°Ñ Ð°Ð±ÑÐ°Ð·Ð¸Ñ
Ð¿Ð¾Ð´Ð²Ð¾Ð´Ð½Ð¾Ðµ Ð±ÐµÑÐ¾Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð¦ÐµÐ»Ñ Ð´Ð¸ÑÑÐµÑÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ - Ð¸Ð·ÑÑÐ¸ÑÑ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼ Ð¸ÑÑÐ¸ÑÐ°Ð½Ð¸Ñ Ð±ÐµÑÐ¾Ð½Ð½ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÑÑ Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ Ð¼Ð¾ÑÑÐºÐ¾Ð¹ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ñ Â«ÐÐµÑÐºÑÑÂ» Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ñ Ð»ÐµÐ´Ð¾Ð²Ð¾Ð¹ Ð°Ð±ÑÐ°Ð·Ð¸Ð¸ Ð¸ Ð²ÑÐ±ÑÐ°ÑÑ Ð»ÑÑÑÐ¸Ð¹ Ð²Ð°ÑÐ¸Ð°Ð½Ñ Ð´Ð»Ñ ÑÐµÐ¼Ð¾Ð½ÑÐ° Ð±ÐµÑÐ¾Ð½Ð½Ð¾Ð¹ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸. ÐÐ±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ - Ð¸ÑÑÐ¸ÑÐ°ÐµÐ¼Ð¾ÑÑÑ Ð±ÐµÑÐ¾Ð½Ð½ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ» Ð¸Ð·ÑÑÐµÐ½ Ð¼ÐµÑÐ°Ð½Ð¸Ð·Ð¼ Ð¸ÑÑÐ¸ÑÐ°Ð½Ð¸Ñ Ð±ÐµÑÐ¾Ð½Ð½ÑÑ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¹, ÑÐ¸Ð¿Ñ ÑÐ¾Ð¾ÑÑÐ¶ÐµÐ½Ð¸Ñ, Ð¿Ð¾Ð´Ð²ÐµÑÐ³Ð°ÑÑÐ¸ÐµÑÑ Ð¸ÑÑÐ¸ÑÐ°Ð½Ð¸Ñ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½ÑÐµ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð·Ð°ÑÐ¸ÑÐµ Ð¾Ñ Ð¸ÑÑÐ¸ÑÐ°Ð½Ð¸Ñ, Ð¸ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð¿ÑÐ¸Ð¼ÐµÑÑ Ð·Ð°ÑÐ¸ÑÑ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½ Ð¼ÐµÑÐ¾Ð´ Ð·Ð°ÑÐ¸ÑÑ Ð¾Ñ Ð»ÐµÐ´Ð¾Ð²Ð¾Ð¹ Ð°Ð±ÑÐ°Ð·Ð¸Ð¸ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ñ Â«ÐÐµÑÐºÑÑÂ». ÐÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½ Ð¼ÐµÑÐ¾Ð´ ÑÐµÐ¼Ð¾Ð½ÑÐ° Ð¶ÐµÐ»ÐµÐ·Ð¾Ð±ÐµÑÐ¾Ð½Ð° Ð½Ð° Ð´Ð°Ð½Ð½Ð¾Ð¹ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ðµ. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½ ÑÐ°ÑÑÑÑ Ð»ÐµÐ´Ð¾Ð²Ð¾Ð¹ Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸ Ð½Ð° ÐºÐ¾Ð»Ð¾Ð½Ð½Ñ Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð»Ð°ÑÑÐ¾ÑÐ¼Ñ, ÑÐ°ÑÑÑÑ Ð²Ð¾Ð»Ð½Ð¾Ð²Ð¾Ð¹ Ð½Ð°Ð³ÑÑÐ·ÐºÐ¸ Ð½Ð° Ð³ÐµÑÐ¼Ð¾ÐºÐ°Ð¼ÐµÑÑ. ÐÐ¾ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ°Ð¼ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ ÑÑÐ¾ÑÐ¼ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð²ÑÐ²Ð¾Ð´Ñ.
I pozzi di Rosetta
Creators: Caterina Boccato
Publisher: name: Media Inaf
Year: 2015

Pubblicata su Nature uno studio sugli ultimi risultati ottenuti grazie a OSIRIS, lo strumento d’imaging a bordo di Rosetta. Spiegato il perché dei “pozzi” presenti sul suolo della cometa Churyumov Gerasimenko
title: ÐÐ¾Ð½ÑÐ¿ÐµÐºÑ Ð»ÐµÐºÑÐ¸Ð¹ Ð¿Ð¾ Ð²ÑÑÑÐµÐ¹ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Â«Ð¢ÐµÑ Ð½Ð¾ÑÑÐµÑÐ½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑÂ». Ð¢ÐµÐ¼Ð°: "ÐÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÑ (Ð´Ð¾ ÑÐ»ÑÑÐ°Ð¹Ð½Ð¾Ð¹ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½Ñ)"
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ°Ð½Ð´Ð°ÐºÑÑÐ¾Ð², ÐÐ³Ð¾ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2021
Subjects: ÐÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐµÐ¹ ÑÐµÐ¾ÑÐ¸Ñ

description: Ð£ÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ Ð¤ÐÐÐ¡ ÐÐ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«ÐÑÑÑÐ°Ñ Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÐºÐ°Â» Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 20.03.01 Â«Ð¢ÐµÑÐ½Ð¾ÑÑÐµÑÐ½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑÂ», Ð¡Ð¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ðµ Ð½ÐµÑÐºÐ¾Ð»ÑÐºÐ¾ ÑÐ¸ÑÐµ, ÑÐµÐ¼ Ð¸Ð·Ð»Ð°Ð³Ð°ÐµÐ¼Ð¾Ðµ Ð½Ð° Ð°ÑÐ´Ð¸ÑÐ¾ÑÐ½ÑÑ Ð·Ð°Ð½ÑÑÐ¸ÑÑ, Ð² Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ ÑÑÐ¾ ÐºÐ°ÑÐ°ÐµÑÑÑ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð²-Ð·Ð°Ð¾ÑÐ½Ð¸ÐºÐ¾Ð² Ð² ÑÐ²ÑÐ·Ð¸ Ñ Ð¼Ð°Ð»ÑÐ¼ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾Ð¼ Ð°ÑÐ´Ð¸ÑÐ¾ÑÐ½ÑÑ ÑÐ°ÑÐ¾Ð². Ð Ð°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð±Ð¾Ð»ÑÑÐ¾Ðµ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð¾ Ð¿ÑÐ¸Ð¼ÐµÑÐ¾Ð², ÑÑÐ¾ Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¿Ð¾Ð»ÐµÐ·Ð½Ð¾ Ð¿ÑÐ¸ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐµ ÐºÐ°Ðº Ðº ÑÐºÐ·Ð°Ð¼ÐµÐ½Ñ, ÑÐ°Ðº Ð¸ Ðº ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½ÑÐ¼ ÑÐ°Ð±Ð¾ÑÐ°Ð¼. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Â«Ð¢ÐµÑÐ½Ð¾ÑÑÐµÑÐ½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑÂ», ÐºÐ°Ðº Ð¾ÑÐ½Ð¾Ð³Ð¾, ÑÐ°Ðº Ð¸ Ð·Ð°Ð¾ÑÐ½Ð¾Ð³Ð¾ Ð¾ÑÐ´ÐµÐ»ÐµÐ½Ð¸Ñ.
L’espansione cosmica verso il Big Rip
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Tre fisici della Vanderbilt University hanno introdotto una nuova formulazione matematica per trattare la dinamica dei fluidi relativistici. Lo studio, pubblicato su Physical Review D, ha delle implicazioni importanti per il destino ultimo dell’Universo e potrebbe far luce allo stesso tempo sulla natura dell’energia oscura. Anche se si tratta di un approccio promettente, occorrerà comunque un'analisi più approfondita per verificare o meno la veridicità dei risultati
La farfalla e lo scorpione
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2015

Un ammasso stellare che ricorda le ali aperte di una farfalla, splendide costellazioni, l'imperdibile congiunzione Venere-Giove e non solo. I consigli per osservare queste e altre meraviglie nel cielo serale del mese appena iniziato
Gli incontri al Teatro del Cielo
Creators: Francesca Brunetti
Publisher: name: Media Inaf
Year: 2015

Conclusa la prima parte di Notti d’Estate ad Arcetri, gli incontri al Teatro del Cielo dell’INAF - Osservatorio Astrofisico di Arcetri, un giugno segnato da una grande partecipazione del pubblico
title: English language extensive reading
title: ÑÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð¿Ð¾ Ð´Ð¾Ð¼Ð°ÑÐ½ÐµÐ¼Ñ ÑÑÐµÐ½Ð¸Ñ
titleType: Subtitle
Creators: name: ÐÐ°Ð»Ð¸ÐµÐ²Ð°, Ð¤Ð°ÑÐ¸Ð¼Ð°
name: ÐÐ°ÑÐ»Ð°Ð¼Ð¾Ð²Ð°, ÐÐµÑÐ°
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2021
Subjects: ÑÑÐµÐ½Ð¸Ðµ
Ð°Ð¼ÐµÑÐ¸ÐºÐ°Ð½ÑÐºÐ°Ñ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ°
ÑÐ°Ð±Ð¾ÑÐ° Ñ ÑÐµÐºÑÑÐ¾Ð¼
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð£ÑÐµÐ±Ð½Ð¾-Ð¼ÐµÑÐ¾Ð´Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¾ Ð½Ð° Ð¾ÑÐ½Ð¾Ð²Ðµ ÑÐ¾Ð¼Ð°Ð½Ð¾Ð² Ð´Ð²ÑÑ Ð°Ð¼ÐµÑÐ¸ÐºÐ°Ð½ÑÐºÐ¸Ñ Ð¿Ð¸ÑÐ°ÑÐµÐ»ÐµÐ¹: Ð¤. Ð¡. Ð¤Ð¸ÑÐ´Ð¶ÐµÑÐ°Ð»ÑÐ´ - Â«ÐÐ¾ÑÑ Ð½ÐµÐ¶Ð½Ð°Â» Ð¸ Ð. Ð¥ÐµÐ¹Ð»Ð¸ - Â«ÐÑÐµÐ»ÑÂ». Ð¦ÐµÐ»ÑÑ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ Ð¾Ð·Ð½Ð°ÐºÐ¾Ð¼Ð»ÐµÐ½Ð¸Ðµ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ñ Ð¾ÑÐ¸Ð³Ð¸Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ Ð°Ð¼ÐµÑÐ¸ÐºÐ°Ð½ÑÐºÐ¾Ð¹ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ¾Ð¹ Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ðµ Ð¸Ñ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð¹ ÐºÐ¾Ð¼Ð¿ÐµÑÐµÐ½ÑÐ¸Ð¹. ÐÐ¾ÑÐ¾Ð±Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÑ Ð·Ð°Ð´Ð°Ð½Ð¸Ð¹ Ð½Ð° Ð¿Ð¾Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÑÐ¸ÑÐ°Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð°ÑÐµÑÐ¸Ð°Ð»Ð°. ÐÑÐ¾Ð±Ð¾Ðµ Ð²Ð½Ð¸Ð¼Ð°Ð½Ð¸Ðµ ÑÐ´ÐµÐ»ÑÐµÑÑÑ Ð°Ð½Ð°Ð»Ð¸ÑÐ¸ÑÐµÑÐºÐ¸Ð¼ ÑÐ¾ÑÐ¼Ð°Ð¼ ÑÐ°Ð±Ð¾ÑÑ Ñ ÑÐµÐºÑÑÐ¾Ð¼, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ°Ð±Ð¾ÑÐµ Ñ Ð»ÐµÐºÑÐ¸ÑÐµÑÐºÐ¸Ð¼Ð¸ ÐµÐ´Ð¸Ð½Ð¸ÑÐ°Ð¼Ð¸. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² 1-2 ÐºÑÑÑÐ¾Ð² Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ¸Ð°ÑÐ°, Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Â«ÐÐ¸Ð½Ð³Ð²Ð¸ÑÑÐ¸ÐºÐ°Â». ÐÐ¾Ð¶ÐµÑ Ð±ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð² ÑÐ°Ð¼ÐºÐ°Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½: Â«Ð§ÑÐµÐ½Ð¸ÐµÂ», Â«ÐÑÐ½Ð¾Ð²Ñ Ð´ÐµÐ»Ð¾Ð²Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐ½Ð¸ÑÂ» Ð¸ Ð´ÑÑÐ³Ð¸Ñ, Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÑÑÐ¸Ñ ÑÐ°Ð±Ð¾ÑÑ Ñ Ð¾ÑÐ¸Ð³Ð¸Ð½Ð°Ð»ÑÐ½ÑÐ¼Ð¸ Ð°Ð½Ð³Ð»Ð¾ÑÐ·ÑÑÐ½ÑÐ¼Ð¸ Ð»Ð¸ÑÐµÑÐ°ÑÑÑÐ½ÑÐ¼Ð¸ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ°Ð¼Ð¸.
Partial Dynamical Symmetry and Anharmonicity in Gamma-Soft Nuclei
Creators: name: Leviatan, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: FOS: Physical sciences

description: Partial dynamical symmetry is shown to be relevant for describing the anharmonicity of excited bands in $^{196}$Pt while retaining solvability and good SO(6) symmetry for the ground band.
description: 4 pages, 1 figure, Proc. Int. Conf. on "Nuclear Structure and Dynamics", May 4-8, 2009, Dubrovnik, Croatia
Nel cuore di un gigante
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2015

Questa splendida veduta variopinta di un gruppo di stelle immerse nelle nubi di gas è stata catturata dalla camera WFI (Wide Field Imager) montata sul telescopio da 2,2 metri dell'MPG/ESO all'Osservatorio dell'ESO di La Silla in Cile. Mostra un ammasso aperto giovane, chiamato NGC 2367, un raggruppamento di stelle neonate al centro di una struttura enorme e molto più antica ai margini della Via Lattea
Valutazione della Ricerca, nuovo via
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2015

Via libera al secondo esercizio di Valutazione della qualità della ricerca (VQR): sotto la 'lente' i lavori prodotti nel quadriennio 2011-2014. Il Ministro dell'Istruzione, dell'Università e della Ricerca Stefania Giannini ha firmato, infatti, il decreto con i criteri di cui l'Anvur, l'Agenzia nazionale incaricata della valutazione, dovrà tenere conto
Come ti misuro l’età delle stelle
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Le osservazioni realizzate da Kepler su un insieme di 33 stelle che ospitano sistemi planetari hanno permesso di calcolare con una precisione elevata l'età delle stelle e altri parametri fondamentali. Lo studio suggerisce che questi oggetti possiedono pianeti di tipo terrestre, il che ci fornisce una chiara indicazione che tali pianeti si siano formati nella Via Lattea molto tempo prima della Terra e si stanno ancora formando. I risultati su Monthly Notices
Galaxy Mergers and Dark Matter Halo Mergers in LCDM: Mass, Redshift, and Mass-Ratio Dependence
Creators: name: Stewart, Kyle R.
name: Bullock, James S.
name: Barton, Elizabeth J.
name: Wechsler, Risa H.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: We employ a high-resolution LCDM N-body simulation to present merger rate predictions for dark matter halos and investigate how common merger-related observables for galaxies--such as close pair counts, starburst counts, and the morphologically disturbed fraction--likely scale with luminosity, stellar mass, merger mass ratio, and redshift from z=0 to z=4. We provide a simple 'universal' fitting formula that describes our derived merger rates for dark matter halos a function of dark halo mass, merger mass ratio, and redshift, and go on to predict galaxy merger rates using number density-matching to associate halos with galaxies. For example, we find that the instantaneous merger rate of m/M>0.3 mass ratio events into typical L > f L* galaxies follows the simple relation dN/dt=0.03(1+f)(1+z)^2.1 Gyr^-1. Despite the rapid increase in merger rate with redshift, only a small fraction of >0.4 L* high-redshift galaxies (~3% at z=2) should have experienced a major merger (m/M >0.3) in the very recent past (t< 100 Myr). This suggests that short-lived, merger-induced bursts of star formation should not contribute significantly to the global star formation rate at early times, in agreement with observational indications. We emphasize that great care must be made in comparisons to observations because the predicted observables depend very sensitively on galaxy luminosity, redshift, overall mass ratio, and uncertain relaxation timescales for merger remnants. We show that the majority of bright galaxies at z=3 should have undergone a major merger (>0.3) in the last 700 Myr and conclude that mergers almost certainly play an important role in delivering baryons and influencing the kinematic properties of Lyman Break Galaxies (LBGs). (abridged)
description: 11 pages, 4 figures, 2 tables; v2 updated to match published version in ApJ. Includes expanded discussion, and fixes typo in "galaxy stellar mass mergers" fitting paramters. Primary results and conclusions unchanged
Il premio Gratton a una tesi sull’alone galattico
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2015

Il premio Livio Gratton, giunto  alla dodicesima edizione, è un premio biennale conferito dall’Associazione Eta Carinae in collaborazione con l’Associazione Tuscolana di Astronomia “Livio Gratton” e l’Associazione Frascati Scienza, con il contributo del Comune di Frascati, e della famiglia Gratton, ed il patrocinio di INAF e del Consiglio Regionale del Lazio
Multiple D$_p$-branes as a D$_{p+2}$-brane
Creators: name: Ali-Akbari, M.
name: Ganjali, M. A.
Publisher: name: arXiv
Year: 2010
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: From BFSS matrix theory considerations, it is expected that a single D$_{p+2}$-brane action can be obtained from N D$_p$-brane action in large N limit. We examine and confirm this expectation by working out the details of DBI and Chern-Simons terms of D$_{p+2}$-brane action from D$_{p}$-brane action. We show that the same relation works for non-BPS, as well as BPS branes
description: 14 pages
Marte low cost
Creators: Davide Coero Borga
Publisher: name: Media Inaf
Year: 2015

Una strategia a lungo termine per raggiungere il Pianeta Rosso: tre scienziati del Jet Propulsion Laboratory e del California Institute of Technology hanno fatto i conti della serva e il budget NASA potrebbe bastare per raggiungere l’obiettivo entro il 2040
Picosecond Ultrasonic Measurements Using an Optical Cavity
Creators: name: Li, Yanqiu
name: Miao, Qian
name: Nurmikko, Arto
name: Maris, Humphrey
Publisher: name: arXiv
Year: 2009
Subjects: subject: Materials Science (cond-mat.mtrl-sci)
subject: FOS: Physical sciences

description: A detailed analysis of the use of an optical cavity to enhance picosecond ultrasonic signals is presented. The optical cavity is formed between a distributed Bragg reflector (DBR) and the metal thin film samples to be studied. Experimental results for Al and Cu films show enhancement of acoustic signals by up to two orders of magnitude and are in good agreement with calculated results based on a previously established model. This technique provides an efficient method for detecting sound in materials with small piezo-optic coefficients and makes it possible to determine the actual pulse shape of the returning acoustic echoes.
description: 30 pages, 13 figures, Picosecond Ultrasonics, Optical Cavity
title: ÐÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿Ð¾Ð³ÑÐµÑÐ½Ð¾ÑÑÐµÐ¹ ÐºÐ»ÑÑÐµÐ²Ð¾Ð³Ð¾ Ð¼ÐµÑÐ¾Ð´Ð° ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¸Ð³Ð½Ð°Ð»Ð° Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½Ð¾-ÑÐ°Ð·Ð¾Ð²Ð¾Ð¹ ÑÐ°Ð´Ð¸Ð¾Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¼Ð°Ð³Ð¸ÑÑÑÐ°
titleType: Subtitle
Creators: name: ÐÐ½Ð°Ð½ÑÐµÐ², ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð Ð°Ð´Ð¸Ð¾Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ½ÑÐµ
Ð£ÑÐ¸Ð»Ð¸ÑÐµÐ»Ð¸ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸
ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÑÑÑÑ Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¸ ÑÐ¿ÐµÐºÑÑÐ°Ð»ÑÐ½ÑÐµ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ° ÑÐ¾ÐºÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¼ÐµÑÐ¾Ð´Ñ ÐµÐ³Ð¾ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ.
Ð¦ÐµÐ»ÑÑ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð²Ð»Ð¸ÑÐ½Ð¸Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÐ¾Ð² Ð¼ÐµÑÐ¾Ð´Ð° ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ° ÑÐ¾ÐºÐ° ÐºÐ»ÑÑÐµÐ²Ð¾Ð³Ð¾ ÑÑÐ¸Ð»Ð¸ÑÐµÐ»Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð½Ð° ÑÐ¾ÑÐ½Ð¾ÑÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¾Ð³Ð¸Ð±Ð°ÑÑÐµÐ¹ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ° ÑÐ¾ÐºÐ° Ð¸ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ð¹ ÑÐ¿ÐµÐºÑÑÐ°Ð»ÑÐ½Ð¾Ð¹ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ¸.
Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð° ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ð° Ð¼Ð¾Ð´ÐµÐ»Ñ ÐºÐ»ÑÑÐµÐ²Ð¾Ð³Ð¾ ÑÑÐ¸Ð»Ð¸ÑÐµÐ»Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÐ¸ Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð° Ð°Ð½Ð°Ð»Ð¸Ð·Ð° ÑÐ°Ð´Ð¸Ð¾Ð½Ð°Ð²Ð¸Ð³Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ ÑÐ¸Ð³Ð½Ð°Ð»Ð°, Ð¾Ð±ÑÐµÐ´Ð¸Ð½ÑÐ½Ð½ÑÐµ Ð² Ð¾Ð´Ð½Ñ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÐ½ÑÑ Ð¼Ð¾Ð´ÐµÐ»Ñ. ÐÑÐ¿Ð¾Ð»ÑÐ·ÑÑ Ð´Ð°Ð½Ð½ÑÑ Ð¼Ð¾Ð´ÐµÐ»Ñ Ð±ÑÐ»Ð¾ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ñ Ð¿Ð°ÑÐ°Ð¼ÐµÑÑÑ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ° ÑÐ¾ÐºÐ°, Ð¿ÑÐ¸ ÐºÐ¾ÑÐ¾ÑÑÑ Ð²ÑÐ¿Ð¾Ð»Ð½ÑÑÑÑÑ ÑÑÐµÐ±Ð¾Ð²Ð°Ð½Ð¸Ñ Ð¿Ð¾ Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐ¼ Ð¸ ÑÐ¿ÐµÐºÑÑÐ°Ð»ÑÐ½ÑÐ¼ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ°Ð¼ Ð¸Ð¼Ð¿ÑÐ»ÑÑÐ°.
title: Ð¢ÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¼ÐµÑ Ð°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÐ°Ð»Â»
title: Ð´Ð¸Ð¿Ð»Ð¾Ð¼Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ
titleType: Subtitle
Creators: name: Ð§ÑÑÐ½Ð¾Ð², ÐÐ¸ÑÐ°Ð»Ð¸Ð¹
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2016
Subjects: ÑÐµÑ Ð½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ
Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ Ð½Ð°Ð»Ð°Ð´ÐºÐ°
Ð±Ð°Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
technological proces
operating adjustment
basing

description: ÐÐ¸Ð¿Ð»Ð¾Ð¼Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ Ð½Ð° ÑÐµÐ¼Ñ: Â«Ð¢ÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ð¹ Ð¿ÑÐ¾ÑÐµÑÑ Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾Ð±ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð´ÐµÑÐ°Ð»Ð¸ Â«ÐÐ°Ð»Â». Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ¾Ð½ÑÑÑÑÐºÑÐ¸Ð¸ Ð´ÐµÑÐ°Ð»Ð¸, Ð²ÑÐ±ÑÐ°Ð½ Ð¼ÐµÑÐ¾Ð´ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð¸ÑÑÐ¾Ð´Ð½Ð¾Ð¹ Ð·Ð°Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸, ÑÐ°ÑÑÑÐ¸ÑÐ°Ð½Ñ Ð¿ÑÐ¸Ð¿ÑÑÐºÐ°, ÑÐµÐ¶Ð¸Ð¼Ñ ÑÐµÐ·Ð°Ð½Ð¸Ñ Ð¸ Ð½Ð¾ÑÐ¼Ñ Ð²ÑÐµÐ¼ÐµÐ½Ð¸ Ð½Ð° Ð²ÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¸Ðµ Ð¾Ð¿ÐµÑÐ°ÑÐ¸Ð¹ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ°. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¿ÑÐ¸ÑÐ¿Ð¾ÑÐ¾Ð±Ð»ÐµÐ½Ð¸Ñ: ÑÑÐ°Ð½Ð¾ÑÐ½Ð¾Ðµ Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½Ð¾-Ð¸Ð·Ð¼ÐµÑÐ¸ÑÐµÐ»ÑÐ½Ð¾Ðµ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐµÑÐ½Ð¸ÐºÐ¸ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸. ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ ÑÐµÑÐ½Ð¸ÐºÐ¾-ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ°.
description: Diploma project on the theme: "Technological process of machining a workpiece "Shaft". In this paper, the analysis of the manufacturability of the design details, selected a method of obtaining metal blanks, the calculated allowance, the cutting conditions and the time allowed for execution of the operations process. Developed fixtures: machining and measuring. Considered safety issues. Performed a feasibility study of the project.
title: ÐÐ±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ðµ Ð¿Ð¾Ð¶Ð°ÑÐ½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ ÑÑÐ´Ð¾Ð²Ð¾Ð³Ð¾ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ñ
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð¤Ð¸ÑÐµÐ½ÐºÐ¾, ÐÐ³Ð¾ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: Ð¿Ð¾Ð¶Ð°ÑÐ½Ð°Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÑ
ÑÑÐ´Ð¾Ð²Ð¾Ðµ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ðµ
Ð²Ð¾Ð·Ð³Ð¾ÑÐ°Ð½Ð¸Ðµ
Ð¼Ð°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ°Ñ Ð¼Ð¾Ð´ÐµÐ»Ñ
ÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ½Ð¾Ðµ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ

description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ Ð¸Ð·Ð»Ð¾Ð¶ÐµÐ½Ð° ÑÑÑÐ½Ð¾ÑÑÑ Ð¿Ð¾Ð»ÐµÐ²Ð¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° Ðº ÑÐ¾Ð·Ð´Ð°Ð½Ð¸Ñ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ Ð¿Ð¾Ð¶Ð°ÑÐ°. ÐÐ»Ñ Ð¸Ð»Ð»ÑÑÑÑÐ°ÑÐ¸Ð¸ Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ ÑÑÐ¾Ð³Ð¾ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð° Ð±ÑÐ»Ð° ÑÐ¾Ð·Ð´Ð°Ð½Ð° 3D-Ð¼Ð¾Ð´ÐµÐ»Ñ Ð²ÐµÑÑÐ½ÐµÐ¹ Ð¿Ð°Ð»ÑÐ±Ñ ÐºÑÐµÐ¹ÑÐµÑÐ° Â«ÐÐ²ÑÐ¾ÑÐ°Â», ÐºÐ¾ÑÐ¾ÑÐ°Ñ Ð²Ð¿Ð¾ÑÐ»ÐµÐ´ÑÑÐ²Ð¸Ð¸ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð»Ð°ÑÑ Ð² ÑÐ¸Ð¼ÑÐ»ÑÑÐ¸Ð¸ Ð¿Ð¾Ð¶Ð°ÑÐ° Ð¿Ð¾ÑÑÐµÐ´ÑÑÐ²Ð¾Ð¼ ÑÐµÑÑÑÑÐ¾Ð² ÑÑÐ¿ÐµÑÐºÐ¾Ð¼Ð¿ÑÑÑÐµÑÐ° Ð¸ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ Fire Dynamics Simulator (FDS). Ð¢Ð°ÐºÐ¶Ðµ Ð±ÑÐ» Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½Ñ Ñ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸ÐµÐ¼ Ð´Ð°ÑÑÐ¸ÐºÐ¾Ð² ÑÐ°Ð·Ð½Ð¾Ð³Ð¾ ÑÐ¸Ð¿Ð°. Ð ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐµ Ð¿ÑÐ¾Ð´ÐµÐ»Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð° Ð´Ð¾ÐºÐ°Ð·Ð°Ð½Ð° ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾ÑÑÑ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¸Ñ Ð´Ð²ÑÑÑÑÐ¾Ð²Ð½ÐµÐ²Ð¾Ð¹ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ°Ð·Ð¼ÐµÑÐµÐ½Ð¸Ñ Ð´Ð°ÑÑÐ¸ÐºÐ¾Ð² Ð² ÑÐµÐ»ÑÑ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð¿Ð¾Ð¶Ð°ÑÐ½Ð¾Ð¹ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ ÑÑÐ´Ð¾Ð²ÑÑ Ð¿Ð¾Ð¼ÐµÑÐµÐ½Ð¸Ð¹.
Piccoli mostri affamati nell’universo vicino
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Le osservazioni effettuate con il telescopio Subaru da un team di scienziati Russi e Giapponesi ci aiutano a far luce sulla natura della classe di sorgenti nota come ultra-luminous X-ray sources, sistemi binari che sembrano ospitare buchi neri molto più piccoli del previsto. I risultati migliorano la nostra comprensione sulla formazione dei buchi neri supermassicci e sul meccanismo di caduta della materia su questi oggetti
Planet formation in highly inclined binaries
Creators: name: Marzari, F.
name: Thebault, P.
name: Scholl, H.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: We explore planet formation in binary systems around the central star where the protoplanetary disk plane is highly inclined with respect to the companion star orbit. This might be the most frequent scenario for binary separations larger than 40 AU, according to Hale (1994). We focus on planetesimal accretion and compute average impact velocities in the habitable region and up to 6 AU from the primary.
description: Accepted for publication on A&A
title: ÐÐ½Ð³Ð»Ð¸Ð¹ÑÐºÐ¸Ðµ Ð¿Ð¾ÑÐ»Ð¾Ð²Ð¸ÑÑ Ð¸ Ð¿Ð¾Ð³Ð¾Ð²Ð¾ÑÐºÐ¸ Ð² Ð°ÐºÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð¼ Ð°ÑÐ¿ÐµÐºÑÐµ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ¸Ð³Ð¾ÑÑÐµÐ²Ð°, ÐÐ»ÐµÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: Ð¿Ð¾ÑÐ»Ð¾Ð²Ð¸ÑÑ
Ð¿Ð¾Ð³Ð¾Ð²Ð¾ÑÐºÐ¸
Ð°ÐºÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸Ñ

description: ÐÐ¸Ð¿Ð»Ð¾Ð¼Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð°ÐºÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð°ÑÐ¿ÐµÐºÑÐ° Ð² Ð¿Ð¾ÑÐ»Ð¾Ð²Ð¸ÑÐ°Ñ Ð¸ Ð¿Ð¾Ð³Ð¾Ð²Ð¾ÑÐºÐ°Ñ Ð°Ð½Ð³Ð»Ð¸Ð¹ÑÐºÐ¾Ð³Ð¾ ÑÐ·ÑÐºÐ°. Ð¦ÐµÐ»ÑÑ ÑÑÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ ÑÐ²Ð»ÑÐµÑÑÑ Ð¾ÑÐ²ÑÑÐ¸ÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±ÑÑÑÐ½ÐµÐ½Ð¸Ðµ Ð°ÐºÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¿Ð¾ÑÐ»Ð¾Ð²Ð¸Ñ Ð¸ Ð¿Ð¾Ð³Ð¾Ð²Ð¾ÑÐ¾Ðº. Ð¡ Ð¿Ð¾Ð¼Ð¾ÑÑÑ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¾Ð² ÑÐ°ÐºÐ¸Ñ ÐºÐ°Ðº Ð¸Ð½ÑÐµÑÐ½ÐµÑ-Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ Ð¸ ÐºÐ½Ð¸Ð³Ð¸ Ð¿Ð¾ Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐµÐ¼Ðµ ÑÐ´ÐµÐ»Ð°Ð½Ñ ÑÐ»ÐµÐ´ÑÑÑÐ¸Ðµ Ð²ÑÐ²Ð¾Ð´Ñ: Ð°ÐºÑÐ¸Ð¾Ð»Ð¾Ð³Ð¸Ñ - ÑÑÐ¾ Ð½Ð°ÑÐºÐ°, Ð¸Ð·ÑÑÐ°ÑÑÐ°Ñ Ð¶Ð¸Ð·Ð½ÐµÐ½Ð½ÑÐµ ÑÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð»ÑÐ´ÐµÐ¹, ÑÐ¾ ÐµÑÑÑ Ð¾Ð½Ð° ÐºÐ°ÑÐ°ÐµÑÑÑ Ð²ÑÐµÐ³Ð¾, ÑÑÐ¾ Ð½Ð°Ñ Ð¾ÐºÑÑÐ¶Ð°ÐµÑ. Ð¡ÑÐ°Ð»Ð¾ ÑÑÐ½Ð¾, ÑÑÐ¾ Ð² ÐºÐ°Ð¶Ð´Ð¾Ð¹ ÐºÑÐ»ÑÑÑÑÐµ ÑÑÑÐµÑÑÐ²ÑÑÑ ÑÐ²Ð¾Ð¸ ÑÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¸, ÑÑÐ¾Ð±Ñ Ð¿Ð¾Ð½ÑÑÑ ÑÐ¾Ñ Ð¸Ð»Ð¸ Ð¸Ð½Ð¾Ð¹ Ð½Ð°ÑÐ¾Ð´, Ð½ÑÐ¶Ð½Ð¾ Ð¸Ð·ÑÑÐ¸ÑÑ ÐµÐ³Ð¾ Ð¸ÑÑÐ¾ÑÐ¸Ñ Ð¸ Ð±ÑÑ. Ð Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ Ð»ÑÐ±Ð¾Ð¹ Ð½Ð°ÑÐ¾Ð´Ð½Ð¾ÑÑÐ¸, Ð² Ð´Ð°Ð½Ð½Ð¾Ð¼ ÑÐ»ÑÑÐ°Ðµ - Ð°Ð½Ð³Ð»Ð¸ÑÐ°Ð½, Ð¿Ð¾Ð¼Ð¾Ð³Ð°ÑÑ Ð¿Ð¾ÑÐ»Ð¾Ð²Ð¸ÑÑ Ð¸ Ð¿Ð¾Ð³Ð¾Ð²Ð¾ÑÐºÐ¸, ÑÐ°Ðº ÐºÐ°Ðº Ð¾Ð½Ð¸ Ð¿ÑÐ¸ÑÐ»Ð¸ Ð¸Ð· Ð´Ð°Ð²Ð½Ð¸Ñ Ð²ÑÐµÐ¼ÐµÐ½ Ð¸ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ñ Ð² ÑÐµÐ±Ðµ Ð¿Ð¾Ð½ÑÑÐ¸Ñ Ð¾ ÑÐµÐ½Ð½Ð¾ÑÑÑÑ. Ð¦ÐµÐ»Ñ ÑÐ°Ð±Ð¾ÑÑ Ð´Ð¾ÑÑÐ¸Ð³Ð½ÑÑÐ° - Ñ Ð¿Ð¾Ð¼Ð¾ÑÑÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ñ Ð±Ð¾Ð»ÑÑÐ¾Ð³Ð¾ ÐºÐ¾Ð»Ð¸ÑÐµÑÑÐ²Ð° Ð¿Ð¾ÑÐ»Ð¾Ð²Ð¸Ñ Ð¸ Ð¿Ð¾Ð³Ð¾Ð²Ð¾ÑÐ¾Ðº Ð²ÑÑÐ²Ð»ÐµÐ½Ñ Ð½ÐµÐºÐ¾ÑÐ¾ÑÑÐµ ÑÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð°Ð½Ð³Ð»Ð¸ÑÐ°Ð½, Ð±Ð¾Ð»ÐµÐµ Ð´ÐµÑÐ°Ð»ÑÐ½Ð¾ Ð¸Ð·ÑÑÐµÐ½ Ð¸Ñ ÑÐ·ÑÐº, Ð¸Ñ ÑÑÐ°Ð´Ð¸ÑÐ¸Ð¸ Ð¸ Ð½ÑÐ°Ð²Ñ.
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° ÐµÐ²ÑÐ¾Ð¿ÐµÐ¹ÑÐºÐ¾Ð¹ ÐºÑÑ Ð½Ð¸ Ð½Ð° 100 Ð¼ÐµÑÑ Ð² ÐÑÐ¸Ð¼Ð¾ÑÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÑÐ°Ð±Ð¾Ð²ÐµÑÐºÐ¸Ð¹, ÐÐ»ÑÑ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2017
Subjects: ÐµÐ²ÑÐ¾Ð¿ÐµÐ¹ÑÐºÐ°Ñ ÐºÑÑ Ð½Ñ
Ð¼ÐµÐ½Ñ
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð°Ñ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÑ
Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð°Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ð°

description: ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐµÑÑÐ¾ÑÐ°Ð½Ð° ÐµÐ²ÑÐ¾Ð¿ÐµÐ¹ÑÐºÐ¾Ð¹ ÐºÑÑÐ½Ð¸ Ð½Ð° 100 Ð¼ÐµÑÑ Ð² ÐÑÐ¸Ð¼Ð¾ÑÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ Ð³. Ð¡Ð°Ð½ÐºÑ - ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°, Ð¿ÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÐµÐ³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸.
title: ÐÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ñ Ð¿ÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²ÐµÐ½Ð½Ð¾-ÑÐ¾ÑÐ³Ð¾Ð²Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐºÐ°ÑÐµ-Ð¿Ð¸ÑÑÐµÑÐ¸Ð¸ Ð½Ð° 50 Ð¼ÐµÑÑ Ð² ÐÐ°ÑÐ¸Ð»ÐµÐ¾ÑÑÑÐ¾Ð²ÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°
title: Ð²ÑÐ¿ÑÑÐºÐ½Ð°Ñ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÐ°
titleType: Subtitle
Creators: name: Ð£ÑÐ¼Ð°Ð½Ð¾Ð², ÐÐ¼Ð¸Ñ
Publisher: name: Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¸Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¸Ð¹ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑ ÐÐµÑÑÐ° ÐÐµÐ»Ð¸ÐºÐ¾Ð³Ð¾
Year: 2018
Subjects: ÐºÐ°ÑÐµ-Ð¿Ð¸ÑÑÐµÑÐ¸Ñ
ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ðµ Ð¾Ð±ÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ
Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ
ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ñ
Ð¼ÐµÐ½Ñ

description: ÐÑÐ¿Ð¾Ð»Ð½ÐµÐ½Ð¾ Ð¼Ð°ÑÐºÐµÑÐ¸Ð½Ð³Ð¾Ð²Ð¾Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð¸Ðµ Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ
ÐºÐ°ÑÐµ-Ð¿Ð¸ÑÑÐµÑÐ¸Ð¸ Ð½Ð° 50 Ð¼ÐµÑÑ Ð² ÐÐ°ÑÐ¸Ð»ÐµÐ¾ÑÑÑÐ¾Ð²ÑÐºÐ¾Ð¼ ÑÐ°Ð¹Ð¾Ð½Ðµ Ð³. Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³Ð°, ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ ÑÐ°ÑÑÐµÑÐ½Ð¾-Ð¿Ð»Ð°Ð½Ð¾Ð²Ð¾Ðµ Ð¼ÐµÐ½Ñ, Ð°ÑÑÐ¾ÑÑÐ¸Ð¼ÐµÐ½Ñ Ð¿ÑÐ¾Ð´ÑÐºÑÐ¸Ð¸ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ°Ñ Ð´Ð¾ÐºÑÐ¼ÐµÐ½ÑÐ°ÑÐ¸Ñ. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°ÑÑÐµÑÑ Ð¾Ð±Ð¾ÑÑÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÑÑÑÑÐºÑÑÑÐ° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ. Ð Ð°Ð·ÑÐ°Ð±Ð¾ÑÐ°Ð½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð±ÐµÐ·Ð¾Ð¿Ð°ÑÐ½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ Ð¿ÑÐ¾ÐµÐºÑÐ¸ÑÑÐµÐ¼Ð¾Ð³Ð¾ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ, ÐµÐ³Ð¾ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ðµ ÑÐµÑÐµÐ½Ð¸Ðµ Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾ÐºÐ°Ð·Ð°ÑÐµÐ»Ð¸.
Risolto il mistero del Litio mancante
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

Osservato per la prima volta da un team internazionale di astronomi il Litio prodotto nell’esplosione di una stella nova: un tassello importante per spiegare l’evoluzione chimica della Via Lattea. Vi hanno contribuito ricercatori INAF di Napoli, Bologna e Trieste
The growth of supermassive black holes in pseudo-bulges, classical bulges and elliptical galaxies
Creators: name: Gadotti, Dimitri A.
name: Kauffmann, Guinevere
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: Using results from structural analysis of a sample of nearly 1000 local galaxies from the Sloan Digital Sky Survey, we estimate how the mass in central black holes is distributed amongst elliptical galaxies, classical bulges and pseudo-bulges, and investigate the relation between their stellar masses and central stellar velocity dispersion sigma. Assuming a single relation between elliptical galaxy/bulge mass, M_Bulge, and central black hole mass, M_BH, we find that 55^{+8}_{-4} per cent of the mass in black holes in the local universe is in the centres of elliptical galaxies, 41^{+4}_{-2} per cent in classical bulges and 4^{+0.9}_{-0.4} per cent in pseudo-bulges. We find that ellipticals, classical bulges and pseudo-bulges follow different relations between their stellar masses and sigma, and the most significant offset occurs for pseudo-bulges in barred galaxies. This structural dissimilarity leads to discrepant black hole masses if single M_BH-M_Bulge and M_BH-sigma relations are used. Adopting relations from the literature, we find that the M_BH-sigma relation yields an estimate of the total mass density in black holes that is roughly 55 per cent larger than if the M_BH-M_Bulge relation is used.
description: 7 pages, 2 figures, accepted for publication in MNRAS main journal after implementing referee's suggestions; results essentially unchanged; main change is to take into account intrinsic scatter in black hole relations
Violation of CP and T in semileptonic decays due to scalar interactions
Creators: name: Castro, G. López
name: López-Lozano, L.
name: Rosado, A.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: Observing charge-parity (CP) or time-reversal (T) violations in the leptonic sector will give useful information to elucidate the nature of neutrinos. CP-violating couplings in charged leptonic currents carry out the weak phases necessary to break these symmetries. Here we study the interference of $W^{\pm}$ and $H^{\pm}$ bosons mediated amplitudes as the origin of possible CP and T violation in semileptonic decays of $K^{\pm}$ mesons and $τ^{\pm}$ leptons. We use the experimental bound on the T-odd transverse polarization asymmetry in $K^+_{μ3}$ decays to predict an upper limit on the CP violating effects in $τ\to K πν$ decays. In the framework of this model with scalar-mediated interactions, we find that current limits on the former process indicate that the CP violating effects in the latter are much smaller than the limits reported so far.
description: 9 pages, 2 figures
Incontro ravvicinato tra Giove e Venere
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

I due corpi celesti più luminosi del Sistema solare (dopo Sole e Luna) si avvicineranno, ai nostri occhi, fino ad una distanza inferiore al diametro della Luna. Il processo è in corso da un mese e la congiunzione sarà visibile dall'Italia domani sera alle 22, puntando i telescopi verso ovest
Effects of Interplanetary Dust on the LISA drag-free Constellation
Creators: name: Cerdonio, Massimo
name: De Marchi, Fabrizio
name: De Pietri, Roberto
name: Jetzer, Philippe
name: Marzari, Francesco
name: Mazzolo, Giulio
name: Ortolan, Antonello
name: Sereno, Mauro
Publisher: name: arXiv
Year: 2010
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: Instrumentation and Methods for Astrophysics (astro-ph.IM)
subject: FOS: Physical sciences

description: The analysis of non-radiative sources of static or time-dependent gravitational fields in the Solar System is crucial to accurately estimate the free-fall orbits of the LISA space mission. In particular, we take into account the gravitational effects of Interplanetary Dust (ID) on the spacecraft trajectories. The perturbing gravitational field has been calculated for some ID density distributions that fit the observed zodiacal light. Then we integrated the Gauss planetary equations to get the deviations from the LISA keplerian orbits around the Sun. This analysis can be eventually extended to Local Dark Matter (LDM), as gravitational fields are expected to be similar for ID and LDM distributions. Under some strong assumptions on the displacement noise at very low frequency, the Doppler data collected during the whole LISA mission could provide upper limits on ID and LDM densities.
description: 11 pages, 6 figures, to be published on the special issue of "Celestial Mechanics and Dynamical Astronomy" on the CELMEC V conference
Quel secondo di troppo
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2015

Martedì 30 giugno durerà 86401 secondi, uno più del solito. Un artificio che si rende periodicamente necessario per compensare il rallentamento della rotazione terrestre. Monia Negusini (INAF): «Lo calcoliamo osservando le quasar con la tecnica VLBI»
Large Charge Four-Dimensional Extremal N=2 Black Holes with R^2-Terms
Creators: name: Gruss, Eyal
name: Oz, Yaron
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Theory (hep-th)
subject: FOS: Physical sciences

description: We consider N=2 supergravity in four dimensions with small R^2 curvature corrections. We construct large charge extremal supersymmetric and non-supersymmetric black hole solutions in all space, and analyze their thermodynamic properties.
description: 18 pages. v2,3: minor fixes
CLIMAAX report Dobrich  First Deliverable
Creators: name: Dobrich Municipality
Publisher: name: Zenodo
Year: 2025

description: Deliverable Phase 1 – Climate risk assessment,  Advanced Risk assessment for ClimAte resilience Debates,Innovations and Actions in Dobrich (ARCADIA), Bulgaria, Dobrich

This report presents the results of the first phase of the climate risk assessment in the Dobrich municipality, focused on flood hazards. The main objective of the analysis is to provide a scientifically sound risk assessment and to serve as a basis for future flood adaptation and management strategies as well as to serve as a pilot analysis for the other climate hazards.

Annex 1 Flood risk assessment, MUNICIPALITY OF DOBRICH
Il primo Asteroid Day
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2015

Se non la fine del mondo, un evento catastrofico causato da un asteroide può essere evitato. L’Asteroid Day vuole proprio sensibilizzare l’opinione pubblica sull’utilità della ricerca e del monitoraggio dei corpi spaziali pericolosi per la Terra, dei quali conosciamo solo l’uno per cento. Tra i sostenitori dell'iniziativa, il musicista e astrofisico Brian May