cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
Transport via coupled states in a C60 peapod quantum dot
Creators: name: Eliasen, Anders
name: Paaske, Jens
name: Flensberg, Karsten
name: Smerat, Sebastian
name: Leijnse, Martin
name: Wegewijs, Maarten R.
name: Jørgensen, Henrik I.
name: Monthioux, Marc
name: Nygård, Jesper
Publisher: name: arXiv
Year: 2010
Subjects: subject: Mesoscale and Nanoscale Physics (cond-mat.mes-hall)
subject: FOS: Physical sciences

description: We have measured systematic repetitions of avoided crossings in low temperature three-terminal transport through a carbon nanotube with encapsulated C60 molecules. We show that this is a general effect of the hybridization of a host quantum dot with an impurity. The well-defined nanotube allows identification of the properties of the impurity, which we suggest to be a chain of C60 molecules inside the nanotube. This electronic coupling between the two subsystems opens the interesting and potentially useful possibility of contacting the encapsulated molecules via the tube.
description: 6 pages, 3 figures
Overview of event-by-event fluctuations
Creators: name: Mrowczynski, Stanislaw
Publisher: name: arXiv
Year: 2009
Subjects: subject: Nuclear Theory (nucl-th)
subject: High Energy Physics - Phenomenology (hep-ph)
subject: Nuclear Experiment (nucl-ex)
subject: FOS: Physical sciences

description: Overview of event-by-event studies on relativistic heavy-ion collisions is given. I focus on fluctuation measurements and on theoretical ideas which appeared experimentally fruitful.
description: 20 pages, 18 figures, presented at the Fourth Workshop on Particle Correlations and Femtoscopy (WPCF2008), Cracow, Poland, September 11-14, 2008
An artifact in fits to conic-based surfaces
Creators: name: Pérez-Escudero, Alfonso
name: Dorronsoro, Carlos
name: Marcos, Susana
Publisher: name: arXiv
Year: 2009
Subjects: subject: Medical Physics (physics.med-ph)
subject: Biological Physics (physics.bio-ph)
subject: Quantitative Methods (q-bio.QM)
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: It is common in Physiological Optics to fit the corneal and the lens surfaces to conic-based surfaces (usually ellipse-based surfaces), obtaining their characteristic radius of curvature and asphericity. Here we show that the variation in radius and asphericity due to experimental noise is strongly correlated. This correlation is seen both in experimental data of the corneal topographer Pentacam and in simulations. We also show that the effect is a characteristic of the geometry of ellipses, and not restricted to any experimental device or fitting procedure.
description: 5 pages, 5 figures
Matteo Renzi in visita al Cern
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2015

Più denaro per il centro di ricerca e uscita delle istituzioni post universitarie dal perimetro del diritto amministrativo. Queste le promesse del premier Matteo Renzi alle ricercatrici e ai ricercatori incontrati oggi a Ginevra. Ferroni (Infn): «La sua presenza qui è per noi motivo d’orgoglio»
title: Ð¤Ð¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¥Ð°Ð½Ð¾Ð²Ð°, ÐÐ°ÑÐ¸Ð½Ð°
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: ÐºÐ°Ð´ÑÐ¾Ð²Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°
ÐºÐ°Ð´ÑÑ
Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»
Ð°Ð´Ð°Ð¿ÑÐ°ÑÐ¸Ñ
Ð½Ð°Ð¹Ð¼ Ð¸ Ð¾ÑÐ±Ð¾Ñ Ð¿ÐµÑÑÐ¾Ð½Ð°Ð»Ð°
Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐµ Ð³Ð¾ÑÑÐ¸Ð½Ð¸ÑÐ½ÑÐµ Ð¾Ð¿ÐµÑÐ°ÑÐ¾ÑÑ
ÑÐµÐ³Ð¼ÐµÐ½Ñ 5*
personnel policy
cadre
personnel
adaptation
the recruitment and selection of staff
international hotel operators
segment 5*

description: Ð¦ÐµÐ»Ñ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ - Ð¿ÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°ÑÑ ÑÑÑÐµÑÑÐ²ÑÑÑÑÑ Ð½Ð° ÐÐÐ Â«ÐÐ Â«ÐÑÑÐ¾ÑÐ¸ÑÂ» ÐºÐ°Ð´ÑÐ¾Ð²ÑÑ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÑ Ñ ÑÐµÐ»ÑÑ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¹ Ð¿Ð¾ ÐµÐµ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ. ÐÑÐµÐ´Ð¼ÐµÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÐºÐ°Ð´ÑÐ¾Ð²Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ° Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð°Ð²ÑÐ¾ÑÐ¾Ð¼ Ð±ÑÐ»Ð¸ ÑÐ°ÑÐºÑÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¸ ÑÑÑÐ½Ð¾ÑÑÑ ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ¸; Ð´Ð°Ð½Ð° Ð¾Ð±ÑÐ°Ñ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÐÐÐ Â«ÐÐ Â«ÐÑÑÐ¾ÑÐ¸ÑÂ». ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ð° ÑÑÑÐµÑÑÐ²ÑÑÑÐ°Ñ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸ ÐºÐ°Ð´ÑÐ¾Ð²Ð°Ñ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐ°; Ð²ÑÑÐ²Ð»ÐµÐ½Ñ ÑÑÑÐµÑÑÐ²ÑÑÑÐ¸Ðµ Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð² ÐºÐ°Ð´ÑÐ¾Ð²Ð¾Ð¹ Ð¿Ð¾Ð»Ð¸ÑÐ¸ÐºÐµ Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ ÐµÐµ ÑÐ¾Ð²ÐµÑÑÐµÐ½ÑÑÐ²Ð¾Ð²Ð°Ð½Ð¸Ñ.
description: The purpose of final qualifying work is to analyze the existing personnel policies at CJSC "GC "Astoria" in order to offer recommendations for its improvement. The subject of research is the personnel policy of the organization. During the work the author has described theoretical basis and essence of the personnel policy; has given a general characteristic of activity of CJSC GK "Astoria". Has analyzed existing company personnel policy and identified existing problems in the personnel policy of the enterprise and measures for its improvement.
C’era una volta una galassia lontana…
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

Utilizzando la tecnica dell'assorbimento dell'idrogeno, un gruppo di ricercatori ha scoperto una galassia lontana ben 5 miliardi di anni. Tutto grazie alle antenne ASKAP, che fanno da apripista a SKA, quello che sarà il network di radiotelescopi più grande del mondo
Cinque mostri sepolti nella polvere
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2015

Il telescopio spaziale NuSTAR ha individuato una popolazione di buchi neri supermassicci fino a oggi invisibili a causa della coltre di gas e polveri che li avvolge. Già se ne sospettava l’esistenza, ma i dati dicono che sono assai più luminosi e attivi del previsto. Anche astronomi INAF fra gli autori della scoperta
title: ÐÐ»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð² Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÑÐµÑÐµ Ð´Ð»Ñ ÑÑÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ (Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐµ ÐÐÐ Â«ÐÐ¸Ð°Ñ Ð¢ÑÑÑÂ»)
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: ÐÐ¸Ð¼ÐµÐ½ÐµÐ·, ÐÑÑÑÐ¸Ð¾
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: ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð°Ñ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ñ
Ð°Ð½Ð°Ð»Ð¸Ð· ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸
Ð¼ÐµÐ´Ð¸Ð°Ð¿Ð»Ð°Ð½

description: ÐÐ¸Ð¿Ð»Ð¾Ð¼Ð½ÑÐ¹ Ð¿ÑÐ¾ÐµÐºÑ ÑÐ¾ÑÑÐ¾Ð¸Ñ Ð¸Ð· Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ñ, ÑÑÐ¸ ÑÐ°Ð·Ð´ÐµÐ»Ð°, Ð¸ Ð¿ÑÐ¸Ð»Ð¾Ð¶ÐµÐ½Ð¸Ð¹. ÐÐ¾ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÑÑÑÑ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð½Ð¾Ð¹ Ðº Ð·Ð°ÑÐ¸ÑÐµ Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ. Ð Ð¿ÐµÑÐ²Ð¾Ð¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²ÑÐ²Ð°ÑÑÑÑ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ½Ð¾Ð²Ñ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ñ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð¾ Ð¾Ð¿Ð¸ÑÐ°Ð½Ð¸Ðµ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ Ð´ÐµÑÑÐµÐ»ÑÐ½Ð¾ÑÑÐ¸ ÑÑÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ Â«ÐÐ¸Ð°Ñ Ð¢ÑÑÑÂ». Ð ÑÑÐµÑÑÐµÐ¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð¿ÑÐ¾Ð²Ð¾Ð´Ð¸ÑÑÑ ÑÐµÐºÐ¾Ð¼ÐµÐ½Ð´Ð°ÑÐ¸Ð¸ Ð¿Ð¾ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸Ðµ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÐºÐ°Ð¼Ð¿Ð°Ð½Ð¸Ð¸ Ð² Ð¸Ð½ÑÐµÑÐ½ÐµÑ-ÑÑÐµÑÐµ Ð´Ð»Ñ ÑÑÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ ÐºÐ¾Ð¼Ð¿Ð°Ð½Ð¸Ð¸ ÐÐÐ Â«ÐÐ¸Ð°Ñ Ð¢ÑÑÑÂ».
Additional file 1 of Changes in individual and contextual socio-economic level influence on reproductive behavior in Spanish women in the MCC-Spain study
Creators: name: Gómez-Acebo, Inés
name: Dierssen-Sotos, Trinidad
name: Palazuelos, Camilo
name: Castaño-Vinyals, Gemma
name: Pérez-Gómez, Beatriz
name: Amiano, Pilar
name: Fernández-Villa, Tania
name: Ardanaz, Eva
name: Suarez-Calleja, Claudia
name: Alguacil, Juan
name: Molina-Barceló, Ana
name: Jiménez-Moleón, José J.
name: Molero, Jessica Alonso
name: Roca-Barceló, Aina
name: Chirlaque, María-Dolores
name: Vázquez, José Pedro Fernández
name: Molinuevo, Amaia
name: Aragonés, Nuria
name: Serra, Maria Sala
name: Binefa, Gemma
name: Moreno, Victor
name: Pollán, Marina
name: Kogevinas, Manolis
name: Llorca, Javier
Publisher: name: figshare
Year: 2020
Subjects: subject: Cell Biology
subject: Biotechnology
subject: Environmental Sciences not elsewhere classified
subject: Sociology
subject: FOS: Sociology
subject: Mathematical Sciences not elsewhere classified
subject: Developmental Biology
subject: Cancer
subject: Science Policy
subject: Mental Health

description: Additional file 1 Supplementary Figure 1. Age at first birth without stratifying by education level. Supplementary Figure 2. Age at first newborn by birth cohort obtained via regression spline. Supplementary Figure 3. Percentage of women with each education level, according to birth cohorts. Supplementary Table 1. Association between socioeconomic scores and quantitative variables. Marginal averages with 95% confidence intervals. Supplementary Table 2. Association between individual and contextual socioeconomic scores with dichotomic variables associated with reproduction. Marginal probabilities of the event occurrence with 95% confidence intervals.
Hyper Velocity Stars and the Restricted Parabolic 3-body Problem
Creators: name: Sari, Re'em
name: Kobayashi, Shiho
name: Rossi, Elena M.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Astrophysical Phenomena (astro-ph.HE)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: Motivated by detections of hypervelocity stars that may originate from the Galactic Center, we revist the problem of a binary disruption by a passage near a much more massive point mass. The six order of magnitude mass ratio between the Galactic Center black hole and the binary stars allows us to formulate the problem in the restricted parabolic three-body approximation. In this framework, results can be simply rescaled in terms of binary masses, its initial separation and binary-to-black hole mass ratio. Consequently, an advantage over the full three-body calculation is that a much smaller set of simulations is needed to explore the relevant parameter space. Contrary to previous claims, we show that, upon binary disruption, the lighter star does not remain preferentially bound to the black hole. In fact, it is ejected exactly in 50% of the cases. Nonetheless, lighter objects have higher ejection velocities, since the energy distribution is independent of mass. Focusing on the planar case, we provide the probability distributions for disruption of circular binaries and for the ejection energy. We show that even binaries that penetrate deeply into the tidal sphere of the black hole are not doomed to disruption, but survive in 20% of the cases. Nor do these deep encounters produce the highest ejection energies, which are instead obtained for binaries arriving to 0.1-0.5 of the tidal radius in a prograde orbit. Interestingly, such deep-reaching binaries separate widely after penetrating the tidal radius, but always approach each other again on their way out from the black hole.[shortened]
description: 10 pages, 10 Figures, Apj submitted
Occhio a Europa
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2015

A prima vista sembra un bulbo oculare, ma in realtà si tratta di una ripresa di Europa, una delle lune di Giove. Quelli che sembrano capillari sanguigni sono in realtà delle profonde fratture e creste che attraversano la crosta ghiacciata del corpo celeste
title: ÐÐ¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð² Ð¸Ð½ÑÐ¾ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼Ð°Ñ . ÐÐµÑÐ¾Ð´Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ ÑÐ»ÑÑÐ°Ð¹Ð½ÑÑ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½ Ð¸ ÑÐ»ÑÑÐ°Ð¹Ð½ÑÑ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð²
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÑÑÐ¸Ñ ÑÑÐµÐ±Ð½ÑÑ Ð·Ð°Ð²ÐµÐ´ÐµÐ½Ð¸Ð¹, Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ ÑÑ Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² "Ð¢ÐµÑ Ð½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°"
titleType: Subtitle
Creators: name: ÐÐµÐ»ÑÐ³Ð¾Ñ, ÐÐ»ÐµÐºÑÐ°Ð½Ð´Ñ
name: ÐÐ¾ÑÐ»Ð¾Ð², ÐÐ½ÑÐ¾Ð½
name: ÐÐ¾Ð¿Ð¾Ð², ÐÐ²Ð³ÐµÐ½Ð¸Ð¹
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2012
Subjects: Ð¡Ð»ÑÑÐ°Ð¹Ð½ÑÐµ Ð²ÐµÐ»Ð¸ÑÐ¸Ð½Ñ
Ð¡Ð»ÑÑÐ°Ð¹Ð½ÑÐµ Ð¿ÑÐ¾ÑÐµÑÑÑ (Ð¼Ð°Ñ.)
ÐÐ°ÑÐµÐ¼Ð°ÑÐ¸ÑÐµÑÐºÐ¾Ðµ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ
Ð Ð°Ð´Ð¸Ð¾ÑÐµÑ Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ

description: Ð¡Ð¸ÑÑÐµÐ¼Ð½ÑÐ¹ Ð¿Ð¾Ð´ÑÐ¾Ð´ Ðº Ð¸Ð¼Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¼Ñ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¿ÑÐµÐ´Ð¿Ð¾Ð»Ð°Ð³Ð°ÐµÑ Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð±Ð¾Ð»ÑÑÐ¾Ð³Ð¾ ÑÐ¸ÑÐ»Ð° Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð², ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÑ Ñ Ð¿Ð¾ÑÑÑÐ¾ÐµÐ½Ð¸ÐµÐ¼ Ð¼Ð¾Ð´ÐµÐ»ÐµÐ¹ ÑÐµÐ°Ð»ÑÐ½ÑÑ ÑÐ¸ÑÑÐµÐ¼ Ð¸ Ð¿ÑÐ¾ÑÐµÑÑÐ¾Ð², Ñ Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð¸ÐµÐ¼ Ð¸Ð¼Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½ÑÑ ÑÐºÑÐ¿ÐµÑÐ¸Ð¼ÐµÐ½ÑÐ¾Ð² Ð¸ Ð¸Ð½ÑÐµÑÐ¿ÑÐµÑÐ°ÑÐ¸ÐµÐ¹ ÑÐµÐ·ÑÐ»ÑÑÐ°ÑÐ¾Ð² Ð¸ Ð´Ñ. Ð Ð¿ÑÐµÐ´Ð»Ð°Ð³Ð°ÐµÐ¼Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¸Ð·ÑÑÐ°ÐµÐ¼ÑÐ¹ ÐºÑÑÐ³ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð² ÑÑÑÐµÑÑÐ²ÐµÐ½Ð½Ð¾ ÑÑÐ¶ÐµÐ½ Ð¸ Ð¾ÑÐ¸ÐµÐ½ÑÐ¸ÑÐ¾Ð²Ð°Ð½, Ð³Ð»Ð°Ð²Ð½ÑÐ¼ Ð¾Ð±ÑÐ°Ð·Ð¾Ð¼, Ð½Ð° Ð¸Ð·ÑÑÐµÐ½Ð¸Ðµ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² ÑÑÐ°ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¸Ð¼Ð¸ÑÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð¼Ð¾Ð´ÐµÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ, Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑÐ¸Ñ ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÐ»ÑÑÐ°Ð¹Ð½ÑÑ Ð¾Ð±ÑÐµÐºÑÐ¾Ð² Ñ Ð·Ð°Ð´Ð°Ð½Ð½ÑÐ¼Ð¸ Ð²ÐµÑÐ¾ÑÑÐ½Ð¾ÑÑÐ½ÑÐ¼Ð¸ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð°Ð¼Ð¸. ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐ·Ð¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸ÑÑÑ Ð¿Ð¾ Ð¼Ð°Ð³Ð¸ÑÑÐµÑÑÐºÐ¾Ð¹ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ðµ Â«Ð¡Ð¸ÑÑÐµÐ¼Ñ Ð¸ ÑÐµÑÐ¸ ÑÐ°Ð´Ð¸Ð¾ÑÐ²ÑÐ·Ð¸ Ð¸ ÑÐ°Ð´Ð¸Ð¾Ð²ÐµÑÐ°Ð½Ð¸ÑÂ» Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¼Ð°Ð³Ð¸ÑÑÑÐ¾Ð² Â«ÐÐ½ÑÐ¾ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½ÑÐµ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¸ Ð¸ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ²ÑÐ·Ð¸Â», Ð¼Ð¾Ð¶ÐµÑ Ð±ÑÑÑ ÑÐ°ÐºÐ¶Ðµ Ð¸ÑÐ¿Ð¾Ð»ÑÐ·Ð¾Ð²Ð°Ð½Ð¾ Ð¿ÑÐ¸ Ð¾Ð±ÑÑÐµÐ½Ð¸Ð¸ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Â«Ð¢ÐµÑÐ½Ð¸ÑÐµÑÐºÐ°Ñ ÑÐ¸Ð·Ð¸ÐºÐ°Â», Â«Ð Ð°Ð´Ð¸Ð¾ÑÐµÑÐ½Ð¸ÐºÐ°Â».
description: ÐÐµÑÐ°ÑÐ°ÐµÑÑÑ Ð¿Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ ÑÐµÐ´Ð°ÐºÑÐ¸Ð¾Ð½Ð½Ð¾-Ð¸Ð·Ð´Ð°ÑÐµÐ»ÑÑÐºÐ¾Ð³Ð¾ ÑÐ¾Ð²ÐµÑÐ° Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³ÑÐºÐ¾Ð³Ð¾ Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¿Ð¾Ð»Ð¸ÑÐµÑÐ½Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ½Ð¸Ð²ÐµÑÑÐ¸ÑÐµÑÐ°.
The role of cluster evolution in disrupting planetary systems and disks: the Kozai mechanism
Creators: name: Parker, Richard J.
name: Goodwin, Simon P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We examine the effects of dynamical evolution in clusters on planetary systems or protoplanetary disks orbiting the components of binary stars. In particular, we look for evidence that the companions of host stars of planetary systems or disks could have their inclination angles raised from zero to between the threshold angles (39.23 degrees and 140.77 degrees) that can induce the Kozai mechanism. We find that up to 20 per cent of binary systems have their inclination angles increased to within the threshold range. Given that half of all extrasolar planets could be in binary systems, we suggest that up to 10 per cent of extrasolar planets could be affected by this mechanism.
description: 5 pages, 4 figures, accepted for publication in MNRAS. References updated
Tristenium Serov & Wilson 1995
Creators: name: Serov, Peter A.
name: Wilson, George D. F.
Publisher: name: Zenodo
Year: 1995
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Stenetriidae
Tristenium

description: Tristenium n.gen. Figs 1C,D, 3B Type species. Tristenium acutirostrum (Miiller, 1991b). Species included. See Table 1. Etymology. Tristenium is a re-arrangement and modification of Stenetrium, and is similar to the name of the second author's son. The gender is neuter. Diagnosis. Head frontal margin with weak lateral and antennal spines, antennal spines rounded and longer than blunt lateral spines. Eyes with circlet of few ocelli. Rostrum with broad base and narrow pointed tip. Antennular flagellum with 3 articles. Antennal article 1 without lateral spine. Maxilliped endopodite distal margin with 3 fan setae. Lateral margins of pereonites rounded; pereonites 1-4 subequal in length, longer than remaining pereonites; most pereonites with only 1 coxal lobe or spine visible in dorsal view. Male pereopod I with broad, robust propodus with denticulate setae and broad blunt teeth on propodal palm; dactylus equal in length to propodal palm; propodal palm terminal seta with small accessory seta and serrate ventral margin. Pleopod 11 protopod distal tip rounded without distal extension; exopod and endopod positioned subapically on medial margin. Appendix masculina elongate, tapering to needle-like stylet with long setae on lateral margin. Pleotelson elongate, with 3 free reduced pleonites; posterolateral spines reduced; postanal region roundly triangular, without posterolateral extensions. Figs lE,F, 3C Remarks. The species of this genus all possess heads with reduced lateral and antennal spines, eyes with few ocelli, narrow triangular rostrums, and appendices masculinae with long needle-like stylets. Although a stylet similar to Stenetrium adrianae occurs in this genus, the long setae on the stylet tip and the differences in the body shape, cephalon shape and the shape of the remaining pleopods clearly distinguish this genus as a separate unit.
description: Published as part of Serov, Peter A. & Wilson, George D. F., 1995, A review of the Stenetriidae (Crustacea: Isopoda: Asellota), pp. 39-82 in Records of the Australian Museum 47 (1) on pages 69-72, DOI: 10.3853/j.0067-1975.47.1995.2, http://zenodo.org/record/4654719
description: {"references": ["Miiller, H. - G., 1991 b. Four new species of shallow-water Asellota from the Gulf of Aden (Crustacea: Isopoda). Senckenbergiana marit. 21: 205 - 214."]}
Laurel, abbiamo un problema!
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2015

Problema risolto per la sonda New Horizons che sabato scorso era entrata in ‘safe mode’ a causa di un’anomalia ma da martedì 7 luglio riprenderà la normale attività scientifica. Meno male, perché mancano solo pochissimi giorni all’incontro ravvicinato con Plutone
Spitzer Observations of Spacecraft Target 162173 (1999 JU3)
Creators: name: Campins, H.
name: Emery, J. P.
name: Kelley, M.
name: Fernandez, Y.
name: Licandro, J.
name: Delbo, M.
name: Barucci, A.
name: Dotto, E.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: FOS: Physical sciences

description: Near-Earth asteroid 162173 (1999 JU3) is the primary target of the Hayabusa-2 sample return mission, and a potential target of the Marco Polo sample return mission. Earth-based studies of this object are fundamental to these missions. We present a mid-infrared spectrum (5-38 microns) of 1999 JU3 obtained with NASA's Spitzer Space Telescope in May 2008. These observations place new constraints on the surface properties of this asteroid. To fit our spectrum we used the near-Earth asteroid thermal model (NEATM) and the more complex thermophysical model (TPM). However, the position of the spin-pole, which is uncertain, is a crucial input parameter for constraining the thermal inertia with the TPM; hence, we consider two pole orientations. In the extreme case of an equatorial retrograde geometry we derive a lower limit to the thermal inertia of 150 J/m^2/K/s^0.5. If we adopt the pole orientation of Abe et al. (2008a) our best-fit thermal model yields a value for the thermal inertia of 700+/-200 J/m^2/K/s^0.5 and even higher values are allowed by the uncertainty in the spectral shape due to the absolute flux calibration. The lower limit to the thermal inertia, which is unlikely but possible, would be consistent with a fine regolith similar to wthat is found for asteroid 433 Eros. However, the thermal inertia is expected to be higher, possibly similar to or greater than that on asteroid 25143 Itokawa. Accurately determining the spin-pole of asteroid 162173 will narrow the range of possible values for its thermal inertia.
description: 4 pages, 2 figures; to be published as a Letter in Astronomy and Astrophysics
title: ÐÐ½Ð°Ð»Ð¸Ð· Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÑ ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹ Ð½Ð° Ð³Ð¾ÑÐ½Ð¾ - Ð¼ÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸ÑÐµÑÐºÐ¾Ð¼ ÐºÐ¾Ð¼Ð±Ð¸Ð½Ð°ÑÐµ Ð¸ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ Ð¿Ð¾ Ð¸Ñ Ð¿ÑÐµÐ´Ð¾ÑÐ²ÑÐ°ÑÐµÐ½Ð¸Ñ
title: Ð±Ð°ÐºÐ°Ð»Ð°Ð²ÑÑÐºÐ°Ñ ÑÐ°Ð±Ð¾ÑÐ°
titleType: Subtitle
Creators: name: Ð¢ÑÐ³Ð¾Ð²Ð°, ÐÐ¸ÐºÑÐ¾ÑÐ¸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: ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½Ð°Ñ ÑÐ¸ÑÑÐ°ÑÐ¸Ñ
Ð³Ð¾ÑÑÑÐ¸Ðµ Ð¶Ð¸Ð´ÐºÐ¾ÑÑÐ¸
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description: ÐÐ¾ Ð²Ð²ÐµÐ´ÐµÐ½Ð¸Ð¸ Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½ Ð¾Ð±ÑÐµÐºÑ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ, Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ñ ÑÐµÐ»Ð¸ Ð¸ Ð·Ð°Ð´Ð°ÑÐ¸, Ð¾Ð±Ð¾ÑÐ½Ð¾Ð²Ð°Ð½Ð° Ð°ÐºÑÑÐ°Ð»ÑÐ½Ð¾ÑÑÑ ÑÐµÐ¼Ñ. Ð Ð¿ÐµÑÐ²Ð¾Ð¹ Ð³Ð»Ð°Ð²Ðµ Ð²ÑÐ¿ÑÑÐºÐ½Ð¾Ð¹ ÐºÐ²Ð°Ð»Ð¸ÑÐ¸ÐºÐ°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÑ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÐµÐ½Ð° ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸ÐºÐ° Ð³Ð¾ÑÐ½Ð¾-Ð¼ÐµÑÐ°Ð»Ð»ÑÑÐ³Ð¸ÑÐµÑÐºÐ¾Ð¹ Ð¾ÑÑÐ°ÑÐ»Ð¸ Ð¸ Ð¸ÑÑÐ»ÐµÐ´ÑÐµÐ¼Ð¾Ð³Ð¾ Ð¾Ð±ÑÐµÐºÑÐ°, Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ð° ÐºÐ»Ð°ÑÑÐ¸ÑÐ¸ÐºÐ°ÑÐ¸Ñ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÑ ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹, ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÑÐ¸ÑÑÐµÐ¼Ð° Ð¿Ð¾ Ð¸Ñ Ð¿ÑÐµÐ´ÑÐ¿ÑÐµÐ¶Ð´ÐµÐ½Ð¸Ñ Ð¸ Ð»Ð¸ÐºÐ²Ð¸Ð´Ð°ÑÐ¸Ð¸ Ð½Ð° Ð¿ÑÐµÐ´Ð¿ÑÐ¸ÑÑÐ¸Ð¸. ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¹ Ð³Ð»Ð°Ð²Ðµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ ÑÑÐµÐ½Ð°ÑÐ¸Ð¸ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ñ Ð¸ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð°Ð²Ð°ÑÐ¸Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹, Ð¿ÑÐ¾Ð²ÐµÐ´ÐµÐ½Ð° Ð¾ÑÐµÐ½ÐºÐ° Ð¿Ð¾ÑÐ°Ð¶Ð°ÑÑÐ¸Ñ ÑÐ°ÐºÑÐ¾ÑÐ¾Ð² Ð¿ÑÐ¸ Ð²Ð¾Ð·Ð½Ð¸ÐºÐ½Ð¾Ð²ÐµÐ½Ð¸Ð¸ ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹. Ð ÑÑÐµÑÑÐµÐ¹ Ð³Ð»Ð°Ð²Ðµ Ð¿ÑÐµÐ´Ð»Ð¾Ð¶ÐµÐ½Ñ Ð¼ÐµÑÐ¾Ð¿ÑÐ¸ÑÑÐ¸Ñ Ð¿Ð¾ Ð¿ÑÐµÐ´ÑÐ¿ÑÐµÐ¶Ð´ÐµÐ½Ð¸Ñ ÑÑÐµÐ·Ð²ÑÑÐ°Ð¹Ð½ÑÑ ÑÐ¸ÑÑÐ°ÑÐ¸Ð¹. ÐÐ°ÐºÐ»ÑÑÐµÐ½Ð¸Ðµ ÑÐ¾Ð´ÐµÑÐ¶Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ Ð²ÑÐ²Ð¾Ð´Ñ Ð¿Ð¾ ÑÐ°Ð±Ð¾ÑÐµ.
ISS: arrivano i rifornimenti con la Progress
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

Il 28 aprile un altro cargo Progress era andato perduto, mentre un altro difetto al vettore (questa volta il razzo Falcon 9) ha causato di recente la perdita della navetta Dragon. L'equipaggio ha tirato un sospiro di sollievo commentando: «è come essere a Natale nel mese di luglio»
Mai visto le onde quantistiche? Ecco il film
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2015

Osservata e “filmata” per la prima volta in modo diretto la natura ondulatoria di molecole d’azoto in rotazione. La tecnica utilizzata apre la strada a nuove possibilità di manipolazioni molecolari al confine fra realtà quantistica e realtà classica. I risultati su Science Advances
Neutron scattering Measurements of the phonon density of states of FeSe$_{1-x}$ superconductors
Creators: name: Phelan, D.
name: Millican, J. N.
name: Thomas, E. L.
name: Leao, J. B.
name: Qiu, Y.
name: Paul, R.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Superconductivity (cond-mat.supr-con)
subject: FOS: Physical sciences

description: Inelastic neutron-scattering experiments have been carried out on polycrystalline samples of the FeSe$_{1-x}$ superconductors. We report the phonon density of states for FeSe$_{1-x}$ with Tc$\approx$8 K. The phonon cutoff frequency is observed around 40 meV. No significant change is observed across the superconducting transition. The measurements support the published first-principles calculations [A. Subedi et al., Phys. Rev. B \textbf{78}, 134514 (2008)].
description: new version with changes
La pulsar e la gigante blu faranno scintille
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2015

Una pulsar sta avvicinandosi alla compagna, una stella gigante che possiede un esteso disco di gas e polveri. Disco che tra meno di tre anni attraverserà. Gli astronomi di tutto il mondo stanno preparando all'evento, per indagare in dettaglio le proprietà dei due oggetti celesti. Il commento di Patrizia Caraveo (INAF)
title: ÐÐ¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ ÑÐµÐ³ÑÐ»Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ ÑÑÐµÑÑ Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð¸ Ñ Ð¾Ð·ÑÐ¹ÑÑÐ²Ð°
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ÑÐµÐ², ÐÐµÐ½Ð¸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¸ÑÐ½Ð¾Ðµ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð¾
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description: ÐÐ±ÑÐµÐºÑÐ¾Ð¼ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ ÑÐ²Ð»ÑÐµÑÑÑ ÑÑÐµÑÐ° Ð¶Ð¸Ð»Ð¸ÑÐ½Ð¾Ð³Ð¾ ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð¸ ÑÐ¾Ð·ÑÐ¹ÑÑÐ²Ð°.
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Dry-matter intake during early phases of growth for subspecies of deer (Odocoileus hemionus)
Creators: name: O'Keefe, James John
Publisher: name: University of British Columbia
Year: 2012

description: Forty-five fawns, representative of races of Odocoileus hemionus columbianus, Odocoileus hemionus sitkensis, and Odocoileus hemionus hemionus were raised together under similar environmental conditions. The daily dry matter intake was recorded for all of the animals for periods of from eight to twelve weeks during the early phases of growth which preceded puberty. It was found that dry matter intake reflected the net energy demands of maintenance and growth. Dry matter intake was also influenced by plane of nutrition, composition and digestibility of the ration, and condition of the animal. Some subspecific differences in growth and nutritional efficiencies were observed. It was shown that dry matter intake during early phases of growth of subspecies of Odocoileus hemionus could be estimated if net energy requirements of the animals and the digestibility coefficient of the ration(s) were known. Knowledge of the pattern of growth in the animal is essential for accurate calculation of the net energy requirements.
title: Ð¡ÑÐ°Ð²Ð½ÐµÐ½Ð¸Ðµ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð½Ð²ÐµÑÑÐ¾ÑÐ¾Ð¼ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð° ÑÐµÐ¼ÐµÐ½ÑÐ½Ð¾Ð¹ Ð¼ÐµÐ»ÑÐ½Ð¸ÑÑ ÑÐ°Ð¼Ð¾Ð¸Ð·Ð¼ÐµÐ»ÑÑÐµÐ½Ð¸Ñ
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§Ð¸Ð¶ÐºÐ¾Ð²Ð°, Ð£Ð»ÑÑÐ½Ð°
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: Ð­Ð»ÐµÐºÑÑÐ¾Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ð¸ Ð²ÐµÐ½ÑÐ¸Ð»ÑÐ½ÑÐµ
Ð­Ð»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ñ Ð²ÐµÐ½ÑÐ¸Ð»ÑÐ½ÑÐµ
ÐÐ¾Ð´ÑÐ»ÑÑÐ¸Ñ
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description: Ð Ð°Ð±Ð¾ÑÐ° Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° ÑÑÐ°Ð²Ð½ÐµÐ½Ð¸Ñ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼Ð¾Ð² ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð½Ð²ÐµÑÑÐ¾ÑÐ¾Ð¼ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð´Ð»Ñ Ð¿Ð¸ÑÐ°Ð½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»Ñ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð° ÑÐµÐ¼ÐµÐ½ÑÐ½Ð¾Ð¹ Ð¼ÐµÐ»ÑÐ½Ð¸ÑÑ ÑÐ°Ð¼Ð¾Ð¸Ð·Ð¼ÐµÐ»ÑÑÐµÐ½Ð¸Ñ Ð¼Ð¾ÑÐ½Ð¾ÑÑÑÑ 630ÐºÐÑ. ÐÐ¾ÑÑÑÐ¾ÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ ÑÐ¸ÑÑÐµÐ¼Ñ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´Ð²ÑÑÑÑÐ¾Ð²Ð½ÐµÐ²ÑÐ¼ Ð¸Ð½Ð²ÐµÑÑÐ¾ÑÐ¾Ð¼ Ð½Ð°Ð¿ÑÑÐ¶ÐµÐ½Ð¸Ñ Ð² Matlab Simulink. ÐÐ¾ÑÑÑÐ¾ÐµÐ½Ð° Ð¿Ð¾Ð»Ð½Ð°Ñ ÑÐ¸ÑÑÐµÐ¼Ð° ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ»ÐµÐºÑÑÐ¾Ð´Ð²Ð¸Ð³Ð°ÑÐµÐ»ÐµÐ¼ Ñ Ð¿Ð¾ÑÑÐ¾ÑÐ½Ð½ÑÐ¼Ð¸ Ð¼Ð°Ð³Ð½Ð¸ÑÐ°Ð¼Ð¸. ÐÑÐ¾Ð¸Ð·Ð²ÐµÐ´ÐµÐ½ Ð°Ð½Ð°Ð»Ð¸Ð· ÑÐ°Ð±Ð¾ÑÑ ÑÐ¾Ð·Ð´Ð°Ð½Ð½ÑÑ ÑÐ¸ÑÑÐµÐ¼ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¸Ð½Ð²ÐµÑÑÐ¾ÑÐ¾Ð¼ Ð² ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐµÐ¶Ð¸Ð¼Ð°Ñ ÑÐ°Ð±Ð¾ÑÑ ÑÐ»ÐµÐºÑÑÐ¾Ð¿ÑÐ¸Ð²Ð¾Ð´Ð°.
Le nuove mappe di materia oscura
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Una survey preliminare del cielo, realizzata con una nuova camera a largo campo installata presso il telescopio giapponese Subaru, ha permesso agli astronomi di rivelare ben 9 concentrazioni di materia oscura. I risultati, pubblicati su Astrophysical Journal, sono confortanti per comprendere il ruolo dell’energia oscura in relazione all’espansione dell’Universo. Il passo successivo sarà quello di ampliare la survey per coprire almeno un migliaio di gradi quadrati di cielo
Hansenium Serov & Wilson 1995
Creators: name: Serov, Peter A.
name: Wilson, George D. F.
Publisher: name: Zenodo
Year: 1995
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Stenetriidae
Hansenium

description: Hansenium n.gen. Type species. Hansenium hanseni (Nobili, 1906). Species included. See Table 1. Etymology. Hansenium is named in honor of H.J. Hansen, who provided the first definitive work on the Stenetriidae early in this century. The gender is neuter. Diagnosis. Head with reduced lateral and antennal spines; antennal spines rounded to pointed, longer than pointed lateral spines. Rostrum short, broad and apically flattened, slightly longer than antennal spines. Antennular flagellum with 8-14 articles. Antennal article 1 lateral spine much reduced or absent. Maxilliped endopodite distal margin with 6 fan setae. Pereonites with angular margins on pereonites 1-4; pereonite 1 longer than remaining pereonites; single and double coxal spines on anterior pereonites. Pereon elongate, anterolateral corners of pereonites 1 and 2 in females with large unfused coxal extensions. Pereopod I with large, robust dactylus twice as long as propodal width; propodus reduced, palm serrate in both sexes, and with large terminal spine in males. Male pereopod I carpus lateral margin extended and serrate. Pleopod 11 appendix masculina elongate with blunt distal tip; tip with ring of cuticular hairs; exopod subapical with large protopodal apical extension. Pleotelson with 2 free pleonites. Pleotelson elongate with prominent posterolateral spines; postanal region smoothly rounded. . Remarks. The genus Hansenium is most closely related to Stenetrium sensu stricto in overall morphology but can be distinguished most prominently by the large, pointed extended carpus that participates in grasping with an elongated dactylus. Hansenium also has large reniform eyes, reduced lateral spines and a broad short rostrum. A correction is made to the nomenclature of the species described as S. caicosensis Kensley & Heard, 1991 by changing it to H. caicosense, in order that the species name is consistent with the gender of the genus, i.e. neuter.
description: Published as part of Serov, Peter A. & Wilson, George D. F., 1995, A review of the Stenetriidae (Crustacea: Isopoda: Asellota), pp. 39-82 in Records of the Australian Museum 47 (1) on pages 72-73, DOI: 10.3853/j.0067-1975.47.1995.2, http://zenodo.org/record/4654719
description: {"references": ["Nobili, G., 1906. Diagnoses preliminaires de Crustaces, Decapodes et Isopodes nouveaux recueillis par M. le Dr. G. Seurat aux iles Touamotou. Bulletin du Museum National d'Histoire Naturelle, le serie 12: 256 - 270.", "Kensley, B. & R. W. Heard, 1991. Studies on the Crustacea of the Turks and Caicos Islands, British West Indies. I. Four new marine isopod crustaceans from the vicinity of Pine Cay. Gulf Research Reports 8 (3): 237 - 246."]}
Analysis of the railway heave induced by soil swelling at a site in southern France
Creators: name: Tang, Anh-Minh
name: Cui, Yu-Jun
name: Trinh, Viet-Nam
name: Szerman, Yahel
name: Marchadier, Gilles
Publisher: name: arXiv
Year: 2009
Subjects: subject: Classical Physics (physics.class-ph)
subject: FOS: Physical sciences

description: In order to better understand the heave observed on the railway roadbed of the French high-speed train (TGV) at Chabrillan in southern France, the swelling behaviour of the involved expansive clayey marl taken from the site by coring was investigated. The aim the study is to analyse the part of heave induced by the soil swelling. First, the swell potential was determined by flooding the soil specimen in an oedometer under its in-situ overburden stress. On the other hand, in order to assess the swell induced by the excavation undertaken during the construction of the railway, a second method was applied. The soil was first loaded to its in situ overburden stress existing before the excavation. It was then flooded and unloaded to its current overburden stress (after the excavation). The swell induced by this unloading was considered. Finally, the experimental results obtained were analyzed, together with the results from other laboratory tests performed previously and the data collected from the field monitoring. This study allowed estimating the heave induced by soil swelling. Subsequently, the part of heave due to landslide could be estimated which corresponds to the difference between the monitored heave and the swelling heave.
Le brillanti stelle di NGC 1333
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2015

Lo studio è stato condotto analizzando sia i dati di Chandra su NGC 1333 che quelli riguardanti il cluster Serpente. Il tutto è stato poi messo a paragone con le osservazioni effettuate sulle giovani stelle della Nebulosa di Orione, il cluster stellare forse più studiato nella nostra galassia
Liocoryphe Serov & Wilson 1995
Creators: name: Serov, Peter A.
name: Wilson, George D. F.
Publisher: name: Zenodo
Year: 1995
Subjects: Biodiversity
Taxonomy
Animalia
Arthropoda
Malacostraca
Isopoda
Stenetriidae
Liocoryphe

description: Liocoryphe n.gen. Figs 1G,H, 3D Type species. Liocoryphe minocula (Menzies & Glynn, 1968). Species included. See Table 1. Etymology. Liocoryphe is derived from the Greek words "lius" meaning smooth, and "coryphe" meaning crown of the head. The name refers to the smooth head of this genus which lacks spines or lateral fields. The gender is feminine. Diagnosis. Head dorsal surface smoothly rounded and frontal margin with no lateral spines, antennal spines rounded and much reduced, shorter than rostrum. Rostrum short, broad, rounded; eyes reduced to small rounded, anterolateral group of ocelli. Antennular flagellum with 4-6 articles. Antennal article 1 without lateral spines. Maxilliped endopodite distal margin with 4 fan setae. Pereonite lateral margins blunt to rounded; double coxal extensions visible on pereonites 2-4, single extensions on pereonites 5-6. Male pereopod I dactylus shorter than propodal palm; propodal palm serrate; carpus ventral margin with large, broad, blunt extension; male pereopod covered in long, dense setae from ischium to propodus. Male pleopod 11 protopod with small pointed apical extension; exopod subapical; appendix masculina elongate with blunt distal tip and subapical row of short, proximally directed cuticular hairs, distal tip narrowed slightly. Pleotelson with 2 free pleonites. Pleotelson longer than wide, smoothly truncated to posterolateral spine then smoothly rounded with no telsonic projection between uropods. Remarks. Liocoryphe is closely related to Hansenium and is distinguished by the males having an extended carpus. This genus gains separate generic status by lacking lateral spines on the head, having a small round group of ocelli, a short blunt rostrum, and a large blunt extension on the carpus that does not participate in grasping with the dactylus.
description: Published as part of Serov, Peter A. & Wilson, George D. F., 1995, A review of the Stenetriidae (Crustacea: Isopoda: Asellota), pp. 39-82 in Records of the Australian Museum 47 (1) on pages 73-76, DOI: 10.3853/j.0067-1975.47.1995.2, http://zenodo.org/record/4654719
description: {"references": ["Menzies, R. J. & P. W. Glynn, 1968. The common marine isopod Crustacea of Puerto Rico. Studies on the Fauna of Cura \" ao and other Caribbean Islands 27: 1 - 133."]}
Via libera: Plutone, sto arrivando!
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2015

Mancano ormai solo una decina di giorni all’incontro tra la sonda New Horizons e il sistema di Plutone. Nessuna nuova luna scoperta, ma nelle ultime immagini del pianeta nano suscitano curiosità delle grandi macchie scure molto regolari. Confermata la presenza di metano ghiacciato
Maximal slicing of D-dimensional spherically-symmetric vacuum spacetime
Creators: name: Nakao, Ken-ichi
name: Abe, Hiroyuki
name: Yoshino, Hirotaka
name: Shibata, Masaru
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: We study the foliation of a $D$-dimensional spherically symmetric black-hole spacetime with $D\ge 5$ by two kinds of one-parameter family of maximal hypersurfaces: a reflection-symmetric foliation with respect to the wormhole slot and a stationary foliation that has an infinitely long trumpet-like shape. As in the four-dimensional case, the foliations by the maximal hypersurfaces have the singularity avoidance nature irrespective of dimensionality. This indicates that the maximal slicing condition will be useful for simulating higher-dimensional black-hole spacetimes in numerical relativity. For the case of D=5, we present analytic solutions of the intrinsic metric, the extrinsic curvature, the lapse function, and the shift vector for the foliation by the stationary maximal hypersurfaces. This data will be useful for checking five-dimensional numerical relativity codes based on the moving puncture approach.
description: 20 pages, 8 figures
Uncertainties in Theoretical HeI Emissivities: HII Regions, Primordial Abundance, and Cosmological Recombination
Creators: name: Porter, R. L.
name: Ferland, G. J.
name: MacAdam, K. B.
name: Storey, P. J.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: A number of recent works in astronomy and cosmology have relied upon theoretical He I emissivities, but we know of no effort to quantify the uncertainties in the atomic data. We analyze and assign uncertainties to all relevant atomic data, perform Monte Carlo analyses, and report standard deviations in the line emissivities. We consider two sets of errors, which we call "optimistic" and "pessimistic." We also consider three different conditions, corresponding to prototypical Galactic and extragalactic H II regions and the epoch of cosmological recombination. In the extragalactic H II case, the errors we obtain are comparable to or larger than the errors in some recent $Y_p$ calculations, including those derived from CMB observations. We demonstrate a systematic effect on primordial abundance calculations; this effect cannot be reduced by observing a large number of objects. In the cosmological recombination case, the errors are comparable to many of the effects considered in recent calculations.
description: 5 pages, 3 figures, accepted to MNRAS Letters
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titleType: Subtitle
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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: ÑÐµÐºÑÑÐµÑÑÑ
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INAF sbarca su ALTRIMONDI
Creators: Caterina Boccato
Publisher: name: Media Inaf
Year: 2015

È on line il primo progetto web in lingua italiana per il pubblico e le scuole dedicato alla ricerca sui Pianeti Extrasolari. A vent’anni dalla scoperta del primo pianeta orbitante attorno a una stella diversa dal Sole il numero degli esopianeti scoperti e studiati è salito vertiginosamente così come il numero di ricercatori italiani impegnati in questo campo.
Probing superfluidity of periodically trapped ultracold atoms in a cavity by transmission spectroscopy
Creators: name: Bhattacherjee, Aranya B.
name: Kumar, Tarun
name: ManMohan
Publisher: name: arXiv
Year: 2009
Subjects: subject: Quantum Gases (cond-mat.quant-gas)
subject: Quantum Physics (quant-ph)
subject: FOS: Physical sciences

description: We study a system of periodic Bose condensed atoms coupled to cavity photons using the input-output formalism. We show that the cavity will either act as a through pass Lorentzian filter when the superfluid fraction of the condensate is minimum or completely reflect the input field when the superfluid fraction is maximum. We show that by monitoring the ratio between the transmitted field and the reflected field, one can estimate the superfluid fraction.
description: 3 pages
La nascita di un pianeta in diretta
Creators: Elisa Nichelli
Publisher: name: Media Inaf
Year: 2015

Grazie ad una lunga campagna osservativa realizzata con il Very Large Telescope in Cile, un gruppo di scienziati ha ottenuto la conferma che il pianeta in orbita attorno alla stella HD 100546 è un giovanissimo gigante gassoso. Il sistema si attesta dunque come un laboratorio senza precedenti per lo studio empirico di pianeti giganti nelle prime fasi della loro formazione. Lo studio pubblicato su Astrophysical Journal
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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Ð¼Ð¸Ð½Ð¾Ð²Ð°, ÐÐ½Ð°ÑÑÐ°ÑÐ¸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: ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½ÑÐ¹ Ð¿ÐµÑÐµÐ²Ð¾Ð´
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description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð¾Ð² ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½ÑÑ ÑÑÐ°ÑÐµÐ¹ Ð¸ Ð½Ð¾Ð²Ð¾ÑÑÐµÐ¹. ÐÑÐ¾Ð²ÐµÐ´ÐµÐ½ ÑÑÐ°Ð²Ð½Ð¸ÑÐµÐ»ÑÐ½ÑÐ¹ Ð°Ð½Ð°Ð»Ð¸Ð· Ð¾ÑÐ¸Ð³Ð¸Ð½Ð°Ð»Ð¾Ð² Ñ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð°Ð¼Ð¸, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿ÐµÑÐµÐ²Ð¾Ð´ÑÐµÑÐºÐ¾Ðµ ÑÐ¾Ð¿Ð¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ Ð¸ÑÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ ÑÐµÐºÑÑÐ° Ñ Ð½ÐµÑÐºÐ¾Ð»ÑÐºÐ¸Ð¼Ð¸ Ð²Ð°ÑÐ¸Ð°Ð½ÑÐ°Ð¼Ð¸ Ð¾Ð¿ÑÐ±Ð»Ð¸ÐºÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð¾Ð² Ð½Ð° ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÑ ÑÐµÑÑÑÑÐ°Ñ. ÐÐ·ÑÑÐµÐ½Ñ ÑÐ°Ð·Ð»Ð¸ÑÐ½ÑÐµ Ð²ÑÐµÐ¼ÐµÐ½Ð½ÑÐµ Ð¿ÐµÑÐ¸Ð¾Ð´Ñ, ÐºÐ¾ÑÐ¾ÑÑÐ¼ Ð¿ÑÐ¸ÑÑÑÐ¸ ÑÐ°Ð·Ð»Ð¸ÑÐ¸Ñ Ð² Ð¿ÐµÑÐµÐ²Ð¾Ð´ÑÐµÑÐºÐ¸Ñ Ð¿Ð¾Ð´ÑÐ¾Ð´Ð°Ñ Ðº Ð¿ÐµÑÐµÐ²Ð¾Ð´Ñ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½ÑÑ Ð¿ÑÐ±Ð»Ð¸ÐºÐ°ÑÐ¸Ð¹. ÐÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð¿ÐµÑÐµÐ²Ð¾Ð´Ð¾Ð² Ð¾Ð¿ÑÐ±Ð»Ð¸ÐºÐ¾Ð²Ð°Ð½Ð½ÑÑ Ð¡ÐÐ, ÐºÐ¾ÑÐ¾ÑÑÐµ Ð²Ð»Ð¸ÑÑÑ Ð½Ð° Ð¸Ð½ÑÐµÑÐ¿ÑÐµÑÐ°ÑÐ¸Ñ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð²Ð½Ð¾Ð¹ ÑÐµÐ»Ð¸ ÑÐ¾Ð¾Ð±ÑÐµÐ½Ð¸Ñ Ð¸ Ð¿Ð¾Ð»ÑÑÐµÐ½Ð¸Ñ Ð¸ÑÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ ÐºÐ¾Ð¼Ð¼ÑÐ½Ð¸ÐºÐ°ÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÑÑÐµÐºÑÐ°.
Meno galassie nell’Universo primordiale
Creators: Corrado Ruscica
Publisher: name: Media Inaf
Year: 2015

Quante galassie deboli siamo in grado di osservare? E' una domanda a cui hanno cercato di rispondere un gruppo di ricercatori della Michigan State University (MSU) attraverso una serie di simulazioni numeriche condotte con i supercomputer. I loro risultati, pubblicati su Astrophysical Journal Letters, suggeriscono che l'Universo delle origini potrebbe essere un luogo poco affollato, implicando che il numero delle galassie più distanti, e più deboli, sia da 10 fino a 100 volte inferiore