cometadata/datacite-rtg-text-other-reclassification-records huggingface dataset:
title: ÐÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ Ð¿ÑÐ¾ÐµÐºÑÐ¾Ð² Ð¸ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ ÐµÐµ ÑÐµÐ°Ð»Ð¸Ð·Ð°ÑÐ¸Ð¸ Ð² ÑÐ¸ÑÑÐ¾Ð²Ð¾Ð¹ ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐµ
Creators: name: ÐÐ¿Ð°ÑÐ¸Ð½, Ð¡.
name: "Ð£Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ Ð² ÑÐºÐ¾Ð½Ð¾Ð¼Ð¸ÐºÐµ: Ð¿ÑÐ¾Ð±Ð»ÐµÐ¼Ñ Ð¸ ÑÐµÑÐµÐ½Ð¸Ñ", Ð½Ð°ÑÑÐ½Ð¾-Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ°Ñ ÐºÐ¾Ð½ÑÐµÑÐµÐ½ÑÐ¸Ñ Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¼ ÑÑÐ°ÑÑÐ¸ÐµÐ¼ (Ð ÐÐ¡ÐâÐ­â2018) (2018; Ð¡Ð°Ð½ÐºÑ-ÐÐµÑÐµÑÐ±ÑÑÐ³)
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2018

description: Ð ÑÑÐ°ÑÑÐµ ÑÐ°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð° ÐºÐ¾Ð½ÑÐµÐ¿ÑÐ¸Ñ Ð¾Ð¿ÑÐ¸Ð¼Ð°Ð»ÑÐ½Ð¾Ð³Ð¾
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ÑÑÑÐ¾Ð¸ÑÐµÐ»ÑÑÑÐ²Ð° Ð¿Ð¾ÐºÐ°Ð·Ð°Ð½Ð¾, ÑÑÐ¾ Ð¿ÑÐ¸Ð¼ÐµÐ½ÐµÐ½Ð¸Ðµ ÑÐ¸ÑÑÐ¾Ð²ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÐµÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÑ Ð´Ð¾ÑÑÐ¸Ð¶ÐµÐ½Ð¸Ñ Ð¿ÑÐ¸ÐµÐ¼Ð»ÐµÐ¼Ð¾Ð¹ Ð´Ð»Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ñ ÑÐµÐ»ÐµÐ¹ Ð´Ð¾ÑÑÐ¾Ð²ÐµÑÐ½Ð¾ÑÑÐ¸ Ð¾ÑÐµÐ½Ð¾Ðº Ð¸ Ð¾ÑÐºÑÑÐ²Ð°ÐµÑ Ð½Ð¾Ð²ÑÐµ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½Ð¾ÑÑÐ¸ Ð´Ð»Ñ ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð³Ð¾ ÑÐ¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ ÑÐ¸ÑÐºÐ°Ð¼Ð¸ Ð¸Ð½Ð²ÐµÑÑÐ¸ÑÐ¸Ð¾Ð½Ð½ÑÑ
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Indagine sul carbonio nel Pittore e nella Balena
Creators: Marco Malaspina
Publisher: name: Media Inaf
Year: 2017

Osservando le righe del carbonio nelle nubi di detriti che circondano due giovani stelle, Beta Pictoris e 49 Ceti, un team di astrofisici giapponesi ha trovato indizi sull’evoluzione dei dischi protoplanetari. Lo studio su Astrophysical Journal Letters
C’è aria pesante intorno a Marte
Creators: Marco Galliani
Publisher: name: Media Inaf
Year: 2017

La sonda Maven della Nasa ha individuato per la prima volta nell’atmosfera di un pianeta differente dalla Terra la presenza di ioni di metalli. Questi elementi chimici deriverebbero dalla disgregazione di polveri interplanetarie e meteoroidi in caduta sul Pianeta rosso
La scienza? La imparo sul web con l’Infn
Creators: Eleonora Cossi
Publisher: name: Media Inaf
Year: 2017

Lanciato nel 2002, il sito dell’Istituto nazionale di fisica nucleare è dedicato alla divulgazione per il mondo della scuola e conta oggi oltre 2000 visitatori al giorno. Tutti i contenuti del sito sono realizzati da esperti ai quali studentesse e studenti possono inviare domande. La nuova versione è online da oggi, martedì 11 aprile
Homomorphisms between fuzzy information systems revisited
Creators: name: Zhu, Ping
name: Wen, Qiaoyan
Publisher: name: arXiv
Year: 2010
Subjects: subject: Artificial Intelligence (cs.AI)
subject: FOS: Computer and information sciences

description: Recently, Wang et al. discussed the properties of fuzzy information systems under homomorphisms in the paper [C. Wang, D. Chen, L. Zhu, Homomorphisms between fuzzy information systems, Applied Mathematics Letters 22 (2009) 1045-1050], where homomorphisms are based upon the concepts of consistent functions and fuzzy relation mappings. In this paper, we classify consistent functions as predecessor-consistent and successor-consistent, and then proceed to present more properties of consistent functions. In addition, we improve some characterizations of fuzzy relation mappings provided by Wang et al.
description: 10 pages
Indizi premonitori per supernove di tipo II
Creators: Eleonora Ferroni
Publisher: name: Media Inaf
Year: 2017

Le supernove a collasso nucleare possono mostrare instabilità molti mesi prima dell’esplosione finale. Il materiale periferico viene infatti espulso in precedenza, formando un denso strato di gas circumstellare. Lo studio su Nature Physics
Modeling Microscopic Chemical Sensors in Capillaries
Creators: name: Hogg, Tad
Publisher: name: arXiv
Year: 2008
Subjects: subject: Robotics (cs.RO)
subject: Biological Physics (physics.bio-ph)
subject: Tissues and Organs (q-bio.TO)
subject: FOS: Computer and information sciences
subject: FOS: Physical sciences
subject: FOS: Biological sciences

description: Nanotechnology-based microscopic robots could provide accurate in vivo measurement of chemicals in the bloodstream for detailed biological research and as an aid to medical treatment. Quantitative performance estimates of such devices require models of how chemicals in the blood diffuse to the devices. This paper models microscopic robots and red blood cells (erythrocytes) in capillaries using realistic distorted cell shapes. The models evaluate two sensing scenarios: robots moving with the cells past a chemical source on the vessel wall, and robots attached to the wall for longer-term chemical monitoring. Using axial symmetric geometry with realistic flow speeds and diffusion coefficients, we compare detection performance with a simpler model that does not include the cells. The average chemical absorption is quantitatively similar in both models, indicating the simpler model is an adequate design guide to sensor performance in capillaries. However, determining the variation in forces and absorption as cells move requires the full model.
description: 14 pages, 8 figures
MOESM18 of Deep sequencing on genome-wide scale reveals the unique composition and expression patterns of microRNAs in developing pollen of Oryza sativa
Creators: name: Wei, Li
name: Yan, Long
name: Wang, Tai
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: Authorsâ original file for figure 5
title: ÐÑÐ¾ÐµÐºÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ðµ Ð¸ Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð¾ ÐºÐ¾ÑÑÐµÐ´Ð¶Ð½Ð¾Ð³Ð¾ Ð¿Ð¾ÑÐµÐ»ÐºÐ° Ð² Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐµ ÐÐ¾Ð¼Ð¸
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¡Ð¾ÑÐ²Ð°ÑÑÐ², ÐÑÑÐµÐ¼
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: ÐºÐ¾ÑÑÐµÐ´Ð¶Ð½ÑÐ¹ Ð¿Ð¾ÑÐµÐ»Ð¾Ðº
Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð°Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ°
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description: Ð Ð´Ð°Ð½Ð½Ð¾Ð¹ ÑÐ°Ð±Ð¾ÑÐµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÑÑÑÑ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð±Ð»Ð°Ð³Ð¾ÑÑÑÑÐ¾Ð¹ÑÑÐ²Ð° Ð¸ Ð¸Ð½Ð¶ÐµÐ½ÐµÑÐ½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸ Ð¿Ð¾ÑÐµÐ»ÐºÐ°, Ð° ÑÐ°ÐºÐ¶Ðµ ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½Ð¾Ð¹ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ð¸ ÐºÐ¾ÑÑÐµÐ´Ð¶Ð°. Ð ÑÐ¾Ð´Ðµ ÑÐ°Ð±Ð¾ÑÑ Ð±ÑÐ»Ð¸ ÑÐµÑÐµÐ½Ñ Ð·Ð°Ð´Ð°ÑÐ¸ Ð¿Ð¾ ÑÐ¾ÑÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð»Ð°Ð½Ð¸ÑÐ¾Ð²Ð¾ÑÐ½Ð¾Ð¹ ÑÑÑÑÐºÑÑÑÑ Ð¿Ð¾ÑÐµÐ»ÐºÐ°, Ð¾ÑÐ³Ð°Ð½Ð¸Ð·Ð°ÑÐ¸Ð¸ ÑÐµÐ»ÑÐµÑÐ° ÑÐµÑÑÐ¸ÑÐ¾ÑÐ¸Ð¸, Ð¾Ð±ÐµÑÐ¿ÐµÑÐµÐ½Ð¸Ñ Ð´Ð¾Ð¶Ð´ÐµÐ²Ð¾Ð³Ð¾ Ð²Ð¾Ð´Ð¾Ð¾ÑÐ²ÐµÐ´ÐµÐ½Ð¸Ñ, Ð¿ÑÐµÐ´ÑÑÐ¼Ð¾ÑÑÐµÐ½Ð¸Ñ Ð·Ð°ÑÐ¸ÑÑ Ð¾Ñ Ð¿Ð¾Ð´ÑÐ¾Ð¿Ð»ÐµÐ½Ð¸Ñ Ð² Ð·Ð¾Ð½Ðµ Ð¿Ð¾Ð²ÑÑÐµÐ½Ð½Ð¾Ð³Ð¾ ÑÑÐ¾Ð²Ð½Ñ Ð³ÑÑÐ½ÑÐ¾Ð²ÑÑ Ð²Ð¾Ð´, Ð° ÑÐ°ÐºÐ¶Ðµ Ð¿Ð¾Ð´Ð±Ð¾ÑÑ Ð²Ð¾Ð·Ð¼Ð¾Ð¶Ð½ÑÑ ÑÐ½ÐµÑÐ³Ð¾ÑÑÑÐµÐºÑÐ¸Ð²Ð½ÑÑ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸Ð¹ Ð´Ð»Ñ Ð´Ð¾Ð¼Ð° Ð½Ð° ÑÑÐ°ÑÑÐºÐµ ÐÐÐ¡, Ð¾Ð±ÐµÑÐ¿ÐµÑÐ¸Ð²Ð°ÑÑÐ¸Ñ ÑÐºÑÐ¿Ð»ÑÐ°ÑÐ°ÑÐ¸Ñ Ð·Ð´Ð°Ð½Ð¸Ñ Ð² ÑÐ¾Ð»Ð¾Ð´Ð½Ð¾Ð¼ ÐºÐ»Ð¸Ð¼Ð°ÑÐµ Ð ÐµÑÐ¿ÑÐ±Ð»Ð¸ÐºÐ¸ ÐÐ¾Ð¼Ð¸.
Una straordinaria galassia ordinaria
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2017

Una galassia piccola e debole come tante, ma scoperta da un team di ricercatori, tra cui Laura Pentericci dell’Inaf, ai confini estremi dell'universo. Il suo studio aiuterà gli astronomi a indagare quali oggetti celesti con la loro radiazione hanno contribuito ad alimentare il processo della reionizzazione cosmica
Spacetime Encodings III - Second Order Killing Tensors
Creators: name: Brink, Jeandrew
Publisher: name: arXiv
Year: 2009
Subjects: subject: General Relativity and Quantum Cosmology (gr-qc)
subject: FOS: Physical sciences

description: This paper explores the Petrov type D, stationary axisymmetric vacuum (SAV) spacetimes that were found by Carter to have separable Hamilton-Jacobi equations, and thus admit a second-order Killing tensor. The derivation of the spacetimes presented in this paper borrows from ideas about dynamical systems, and illustrates concepts that can be generalized to higher- order Killing tensors. The relationship between the components of the Killing equations and metric functions are given explicitly. The origin of the four separable coordinate systems found by Carter is explained and classified in terms of the analytic structure associated with the Killing equations. A geometric picture of what the orbital invariants may represent is built. Requiring that a SAV spacetime admits a second-order Killing tensor is very restrictive, selecting very few candidates from the group of all possible SAV spacetimes. This restriction arises due to the fact that the consistency conditions associated with the Killing equations require that the field variables obey a second-order differential equation, as opposed to a fourth-order differential equation that imposes the weaker condition that the spacetime be SAV. This paper introduces ideas that could lead to the explicit computation of more general orbital invariants in the form of higher-order Killing Tensors.
description: 9 pages
Adotta il Pianeta
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2017

Festeggiare la giornata mondiale per la Terra, occasione in cui tutti i cittadini del mondo si uniscono per celebrare il Pianeta e promuoverne la salvaguardia, osservandola dallo spazio. Come? Con una piattaforma dedicata da cui è possibile “adottare” un pezzettino del nostro pianeta e tenerne d’occhio i parametri ambientali. L’Earth Day si celebra ogni anno un mese e due giorni dopo l'equinozio di primavera, il 22 aprile. Quest’anno giunge alla sua 37esima edizione, e l’Inaf c’è
Rate and nature of false positives in the CoRoT exoplanet search
Creators: name: Almenara, J. M.
name: Deeg, H. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Earth and Planetary Astrophysics (astro-ph.EP)
subject: Solar and Stellar Astrophysics (astro-ph.SR)
subject: FOS: Physical sciences

description: Context. The CoRoT satellite searches for planets by applying the transit method, monitoring up to 12 000 stars in the galactic plane for 150 days in each observation run. This search is contaminated by a large fraction of false positives, caused by different binary configurations that might be confused with a transiting planet. Aims. We evaluate the rates and nature of false positives in the CoRoT exoplanets search and compare our results with semiempirical predictions. Methods. We consider the detected binary and planet candidates in the first three extended CoRoT runs, and classify the results of the follow-up observations completed to verify their planetary nature. We group the follow-up results into undiluted binaries, diluted binaries, and planets and compare their abundances with predictions from the literature. Results. 83% of the initial detections are classified as false positives using only the CoRoT light-curves, the remaining 17% require follow-up observations. Finally, 12% of the follow-up candidates are planets. The shape of the overall distribution of the false positive rate follows previous predictions, except for candidates with transit depths below about 0.4%. For candidates with transit depths in the range from 0.1 - 0.4%, CoRoT detections are nearly complete, and this difference from predictions is probably real and dominated by a lower than expected abundance of diluted eclipsing binaries.
description: accepted for A&A special issue on CoRoT
title: ÐÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ðµ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð¾ Ð Ð¾ÑÑÐ¸Ð¸ Ð¸ ÐÐ¸ÑÐ°Ñ Ð² Ð±Ð¾ÑÑÐ±Ðµ Ñ ÑÐµÑÑÐ¾ÑÐ¸Ð·Ð¼Ð¾Ð¼
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ÑÐ¸Ð»Ð¸Ð½, 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: 2016
Subjects: ÑÐ¾ÑÑÐ¸Ð¹ÑÐºÐ¾-ÐºÐ¸ÑÐ°Ð¹ÑÐºÐ¾Ðµ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ð¾
ÑÐµÑÑÐ¾ÑÐ¸Ð·Ð¼
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Russian-Chinese cooperation
terrorism
international terrorism
the fight against terrorism

description: ÐÐ°Ð½Ð½Ð°Ñ ÑÐ°Ð±Ð¾ÑÐ° Ð² Ð¿ÐµÑÐ²ÑÑ Ð¾ÑÐµÑÐµÐ´Ñ Ð¿Ð¾ÑÐ²ÑÑÐµÐ½Ð° Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð¼Ñ ÑÐ¾ÑÑÑÐ´Ð½Ð¸ÑÐµÑÑÐ²Ñ Ð Ð¾ÑÑÐ¸Ð¸ Ñ ÐÐ¸ÑÐ°ÐµÐ¼ Ð² Ð°Ð½ÑÐ¸ÑÐµÑÑÐ¾ÑÐ¸ÑÑÐ¸ÑÐµÑÐºÐ¾Ð¹ Ð±Ð¾ÑÑÐ±Ðµ. ÐÑÐ¾Ð°Ð½Ð°Ð»Ð¸Ð·Ð¸ÑÐ¾Ð²Ð°Ð½Ñ Ð¸ÑÑÐ¾ÑÐ½Ð¸ÐºÐ¸ Ð¿Ð¾ Ð¸ÑÑÐ»ÐµÐ´Ð¾Ð²Ð°Ð½Ð¸Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÐ¾Ð² Ð¾ Ð¿ÑÐ¸ÑÐ¾Ð´Ðµ, Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÑÑ Ð¸ ÑÐ¾ÑÐ¼Ð°Ñ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ ÑÐµÑÑÐ¾ÑÐ¸Ð·Ð¼Ð°. Ð¢Ð°ÐºÐ¶Ðµ Ð² ÑÐ°Ð±Ð¾ÑÐµ Ð¾ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸Ð·Ð¾Ð²Ð°Ð½Ð¾ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ðµ ÑÐ¾ÑÑÐ¾ÑÐ½Ð¸Ðµ ÑÐ¸ÑÑÐµÐ¼Ñ Ð±Ð¾ÑÑÐ±Ñ Ñ ÑÐµÑÑÐ¾ÑÐ¸Ð·Ð¼Ð¾Ð¼ Ð² Ð Ð¾ÑÑÐ¸Ð¸ Ð¸ ÐÐ¸ÑÐ°Ðµ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð±Ð¾ÑÑÐ±Ñ Ñ ÑÐµÑÑÐ¾ÑÐ¸Ð·Ð¼Ð¾Ð¼ ÐºÐ°Ðº ÑÑÑÐ°ÑÐµÐ³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð´Ð²ÑÑÑÑÐ¾ÑÐ¾Ð½Ð½ÐµÐ³Ð¾ Ð¸ Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½Ð¾Ð³Ð¾ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð Ð¾ÑÑÐ¸Ð¸ Ð¸ ÐÐ¸ÑÐ°Ñ. ÐÑÑÐ²Ð»ÐµÐ½Ñ Ð¿ÐµÑÑÐ¿ÐµÐºÑÐ¸Ð²Ð½ÑÐµ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸Ñ Ð Ð¾ÑÑÐ¸Ð¸ Ð¸ ÐÐ¸ÑÐ°Ñ Ð² Ð±Ð¾ÑÑÐ±Ðµ Ñ ÑÐµÑÑÐ¾ÑÐ¸Ð·Ð¼Ð¾Ð¼.
description: This work is primarily devoted to the international cooperation of Russia with China in the fight against terrorism. Analyzed sources for the study of questions about the nature, characteristics and forms of international terrorism. The work also describes the contemporary state system of fight against terrorism in Russia and China. The peculiarities of counter-terrorism as strategic areas of bilateral and international cooperation between Russia and China. Identified prospective directions of interaction of Russia and China in fighting against terrorism.
Gieysztoria chiqchi Damborenea, Brusa & Norena 2005
Creators: name: Braccini, João A. L.
name: Brusa, Francisco
name: Leal-Zanchet, Ana M.
Publisher: name: Zenodo
Year: 2017
Subjects: Biodiversity
Taxonomy
Animalia
Platyhelminthes
Rhabditophora
Rhabdocoela
Dalyelliidae
Gieysztoria
Gieysztoria chiqchi

description: Gieysztoria chiqchi Damborenea, Brusa & Noreña, 2005 Figs 12–13A, B General morphology. Ovoid body (to 1 mm), whitish with dark spots; anterior tip truncated and posterior tip pointed (Figs 12, 13A). Mouth located antero-ventrally; pharynx barrel-shaped. Male copulatory organ with sclerotized stylet, about 170 µm long, with a completely fibrous girdle and 10 spines of different sizes (Fig. 13B). The arrangement, number, and size of spines of the sclerotized stylet, as well as the morphology of its fibrous girdle are identical to these of the type specimens. Specimens examined. MZU 00207: coll. J.A.L. Braccini and F. Brusa, 26 March 2012, Brazil, Rio Grande do Sul, Capivari do Sul (30°10ʹ22ʺ S, 050°23ʹ10ʺ W); coll. J. A. L. Braccini and G. G. Iturralde, 27 September 2012, Brazil, Rio Grande do Sul, Osório (Wetland 2) (29°53ʹ20ʺ S, 050°08ʹ09ʺ W). Remarks on ecology and distribution. This species had a high abundance in the summer/autumn survey, but most of them were dead during the sample analysis, probably due to some disturbance shortly before the survey in Capivari do Sul. It showed low abundance in the summer/ autumn survey in Osório (Table 2). Gieysztoria chiqchi was previously recorded only for its type locality, in the department of Loreto, Peruvian Amazon (Damborenea et al. 2005). Thus, the present record is the first for Brazil and represents an increase of the known distribution of this species of about 3800 km to the southeast.
description: Published as part of João A. L. Braccini, Francisco Brusa & Ana M. Leal-Zanchet, 2017, Six freshwater microturbellarian species (Platyhelminthes) in permanent wetlands of the Coastal Plain of southern Brazil: new records, abundance, and distribution, pp. 849-855 in Check List 13 (6) on page 854, DOI: 10.15560/13.6.849, http://zenodo.org/record/1067944
description: {"references": ["Damborenea C, Brusa F, Norena C (2005) New species of Gieysztoria (Platyhelminthes: Rhabdocoela) from Peruvian Amazon floodplain with description of their stylet ultrastructure. Zoological Science 22: 1319 - 1329. https: // doi. org / 10.2108 / zsj. 22.1319"]}
Scattered X-rays in Obscured Active Galactic Nuclei and their Implications for Geometrical Structure and Evolution
Creators: name: Noguchi, Kazuhisa
name: Terashima, Yuichi
name: Ishino, Yukiko
name: Hashimoto, Yasuhiro
name: Koss, Michael
name: Ueda, Yoshihiro
name: Awaki, Hisamitsu
Publisher: name: arXiv
Year: 2010
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We construct a new sample of 32 obscured active galactic nuclei (AGNs) selected from the Second XMM-Newton Serendipitous Source Catalogue to investigate their multiwavelength properties in relation to the "scattering fraction", the ratio of the soft X-ray flux to the absorption-corrected direct emission. The sample covers a broad range of the scattering fraction (0.1%-10%). A quarter of the 32 AGNs have a very low scattering fraction (smaller than 0.5%), which suggests that they are buried in a geometrically thick torus with a very small opening angle. We investigate correlations between the scattering fraction and multiwavelength properties. We find that AGNs with a small scattering fraction tend to have low [O III]lambda5007/X-ray luminosity ratios. This result agrees with the expectation that the extent of the narrow-line region is small because of the small opening angle of the torus. There is no significant correlation between scattering fraction and far-infrared luminosity. This implies that a scale height of the torus is not primarily determined by starburst activity. We also compare scattering fraction with black hole mass or Eddington ratio and find a weak anti-correlation between the Eddington ratio and scattering fraction. This implies that more rapidly growing supermassive black holes tend to have thicker tori.
description: 13 pages, 10 figures, accepted for publication in ApJ
Local recreational resources for the aged : a comparative survey of two Vancouver districts (1957-8)
Creators: name: Andresson, Edda
Publisher: name: University of British Columbia
Year: 2012

description: The increasing number of persons surviving into old age, the prolongation of the period spent in retirement, and the social changes resulting from urbanization and industrialization, have all combined to make the use of leisure time by the senior citizens an urgent social problem. For this study, two districts from the City of Vancouver, both of which had a high proportion of senior citizens, were selected and compared. The purpose was to assess the effectiveness of existing resources in meeting, the recreational needs of the senior citizens in the two areas. Foremost was the question of the nature of existing resources, their availability to the general population, and. their availability to senior citizens. It also attempted to throw some light on the meaning of recreation to the older person, and the extent to which he is willing or able to involve himself in meeting his own recreational needs. For the purpose of gaining information the cooperation was sought from ministers of local churches, and pensioners' organizations, through the use of questionnaires. These were followed up by personal interviews with staff of social and recreational agencies, representative men and women, and interested citizens. The socio-economic characteristics of the two areas are described, and the recreational resources available and. the use made of them by old people are analyzed. Many groups that replied indicated that the provision of recreation was part of their purpose, but that social action was their primary concern. The questionnaire was useful, but to determine the needs that are considered important by the recreation authorities and the pensioners, it was necessary to make further inquiries through personal interviews with people concerned with the issue. These findings are that the programmes studied are able to meet with varying degrees of success the needs of the senior citizens for companionship with their own group. The extension of existing facilities and programmes, and more frequent meetings are needed, however, to satisfy the emotional and leisure-time needs of senior citizens. In the last chapter, the recreational resources and needs are reviewed and the limitations of the survey are discussed. It appears that the survey dealt primarily with older people of limited financial means who enjoy sufficiently good health to go out to meetings. Larger questions regarding the recreational needs and resources available to all senior citizens, would require further surveys to answer them properly.
Homotopy groups and twisted homology of arrangements
Creators: name: Randell, Richard
Publisher: name: arXiv
Year: 2008
Subjects: subject: Geometric Topology (math.GT)
subject: FOS: Mathematics
subject: 57N65

description: Recent work of M. Yoshinaga shows that in some instances certain higher homotopy groups of arrangements map onto non-resonant homology. This is in contrast to the usual Hurewicz map to untwisted homology, which is always the zero homomorphism in degree greater than one. In this work we examine this dichotomy, generalizing both results.
description: Revised version, to appear in Algebraic & Geometric Topology
«Fletto i muscoli e sono nel vuoto!»
Creators: Redazione Asi
Publisher: name: Media Inaf
Year: 2017

Cosa ci fa quello strano ”astronauta” con la faccia da scimmia e le orecchie da topo sulla Stazione spaziale? Di sicuro niente di buono... Panini Comics presenta ”C’è spazio per tutti”, un evento editoriale firmato Leo Ortolani e realizzato con l’Asi in collaborazione con l’Esa
title: Ð¢ÐµÐ¾ÑÐ¸Ñ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¼Ð½Ð¾Ð³Ð¾ÑÐµÐ»ÐµÐ²ÑÑ Ð³ÑÑÐµÐ½Ð¸ÑÐ½ÑÑ Ð¸ ÐºÐ¾Ð»ÐµÑÐ½ÑÑ Ð¼Ð°ÑÐ¸Ð½. Ð¢ÑÐ³Ð¾Ð²ÑÐ¹ ÑÐ°ÑÑÐµÑ ÐºÑÐ¸Ð²Ð¾Ð»Ð¸Ð½ÐµÐ¹Ð½Ð¾Ð³Ð¾ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² Ð²ÑÐ·Ð¾Ð², Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ñ ÑÑ Ð¿Ð¾ ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÐ¸ âÐÐ²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ðµ- Ð¸ ÑÑÐ°ÐºÑÐ¾ÑÐ¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµâ
titleType: Subtitle
Creators: name: Ð¨ÐµÐ»Ð¾Ð¼Ð¾Ð², ÐÐ»Ð°Ð´Ð¸Ð¼Ð¸Ñ
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ ÐÐ¾Ð»Ð¸ÑÐµÑÐ½. ÑÐ½-ÑÐ°
Year: 2013
Subjects: ÐÐ¾Ð»ÐµÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ
ÐÑÑÐµÐ½Ð¸ÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ

description: Ð¡Ð¾Ð¾ÑÐ²ÐµÑÑÑÐ²ÑÐµÑ ÑÐ¾Ð´ÐµÑÐ¶Ð°Ð½Ð¸Ñ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ñ Ð¡Ð.11 âÐ¢ÐµÐ¾ÑÐ¸Ñ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð³ÑÑÐµÐ½Ð¸ÑÐ½ÑÑ Ð¼Ð°ÑÐ¸Ð½â Ð³Ð¾ÑÑÐ´Ð°ÑÑÑÐ²ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð¾Ð±ÑÐ°Ð·Ð¾Ð²Ð°ÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÑÐ°Ð½Ð´Ð°ÑÑÐ° Ð¿Ð¾ Ð½Ð°Ð¿ÑÐ°Ð²Ð»ÐµÐ½Ð¸Ñ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ 653200 âÐ¢ÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÐµ Ð¼Ð°ÑÐ¸Ð½Ñ Ð¸ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½Ð¾Â­ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÐºÐ¾Ð¼Ð¿Ð»ÐµÐºÑÑâ, ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½Ð¾ÑÑÑ 190201 âÐÐ²ÑÐ¾Ð¼Ð¾Ð±Ð¸Ð»Ðµ- Ð¸ ÑÑÐ°ÐºÑÐ¾ÑÐ¾ÑÑÑÐ¾ÐµÐ½Ð¸Ðµâ. Ð Ð°ÑÑÐ¼Ð¾ÑÑÐµÐ½Ñ Ð²Ð¾Ð¿ÑÐ¾ÑÑ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¿Ð¾Ð²Ð¾ÑÐ¾ÑÐ° Ð±ÑÑÑÑÐ¾ÑÐ¾Ð´Ð½ÑÑ ÑÑÐ°Ð½ÑÐ¿Ð¾ÑÑÐ½ÑÑ Ð³ÑÑÐµÐ½Ð¸ÑÐ½ÑÑ Ð¼Ð°ÑÐ¸Ð½. ÐÑÑÐ°Ð¶ÐµÐ½Ñ ÐºÐ°Ðº ÐºÐ»Ð°ÑÑÐ¸ÑÐµÑÐºÐ¸Ðµ ÑÐ°Ð·Ð´ÐµÐ»Ñ ÑÐµÐ¾ÑÐ¸Ð¸ Ð¿Ð¾Ð²Ð¾ÑÐ¾ÑÐ°, ÑÐ°Ðº Ð¸ Ð¾ÑÐ¸Ð³Ð¸Ð½Ð°Ð»ÑÐ½ÑÐµ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ Ð°Ð²ÑÐ¾ÑÐ°. Ð¢ÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ°Ñ ÑÐ°ÑÑÑ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð¿ÑÐ¾Ð¸Ð»Ð»ÑÑÑÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð° Ð¿ÑÐ¸Ð¼ÐµÑÐ°Ð¼Ð¸ Ð¸ ÑÐ½Ð°Ð±Ð¶ÐµÐ½Ð° Ð·Ð°Ð´Ð°ÑÐ°Ð¼Ð¸ Ð´Ð»Ñ ÑÐ°Ð¼Ð¾ÑÑÐ¾ÑÑÐµÐ»ÑÐ½Ð¾Ð³Ð¾ ÑÐµÑÐµÐ½Ð¸Ñ.ÐÑÐµÐ´Ð½Ð°Ð·Ð½Ð°ÑÐµÐ½Ð¾ Ð´Ð»Ñ ÑÑÑÐ´ÐµÐ½ÑÐ¾Ð² ÑÑÐ°ÑÑÐ¸Ñ ÐºÑÑÑÐ¾Ð², Ð° ÑÐ°ÐºÐ¶Ðµ Ð´Ð»Ñ Ð¿ÑÐµÐ¿Ð¾Ð´Ð°Ð²Ð°ÑÐµÐ»ÐµÐ¹, Ð¿ÑÐ¾Ð²Ð¾Ð´ÑÑÐ¸Ñ Ð¿ÑÐ°ÐºÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð·Ð°Ð½ÑÑÐ¸Ñ. ÐÐ¾Ð¶ÐµÑ ÑÐ°ÐºÐ¶Ðµ Ð¿ÑÐµÐ´ÑÑÐ°Ð²Ð»ÑÑÑ Ð¸Ð½ÑÐµÑÐµÑ Ð´Ð»Ñ Ð»ÑÐ±Ð¸ÑÐµÐ»ÐµÐ¹ ÑÐµÑÐ½Ð¸ÐºÐ¸, ÐºÐ¾ÑÐ¾ÑÑÐµ ÑÐ¾ÑÑÑ ÑÐ°ÑÑÐ¸ÑÐ¸ÑÑ ÑÐ²Ð¾Ð¹ ÐºÑÑÐ³Ð¾Ð·Ð¾Ñ Ð² Ð¾Ð±Ð»Ð°ÑÑÐ¸ ÑÐµÐ¾ÑÐ¸Ð¸ Ð´Ð²Ð¸Ð¶ÐµÐ½Ð¸Ñ Ð¸ Ð¼ÐµÑÐ¾Ð´Ð¾Ð² Ð¾Ð¿ÑÐµÐ´ÐµÐ»ÐµÐ½Ð¸Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÑ ÑÐ°ÑÐ°ÐºÑÐµÑÐ¸ÑÑÐ¸Ðº Ð³ÑÑÐµÐ½Ð¸ÑÐ½ÑÑ Ð¼Ð°ÑÐ¸Ð½.
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°.
Tree-level contributions to the rare decays B+ --> pi+ nu anti-nu, B+ --> K+ nu anti-nu, and B+ --> K*+ nu anti-nu in the Standard Model
Creators: name: Kamenik, Jernej F.
name: Smith, Christopher
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Phenomenology (hep-ph)
subject: FOS: Physical sciences

description: The tree-level contributions to the rare decays B+ --> pi+ nu anti-nu, B+ --> K+ nu anti-nu, and B+ --> K*+ nu anti-nu are analyzed and compared to those occurring in K+ --> pi+ nu anti-nu, D+ --> pi+ nu anti-nu, and Ds+ --> pi+ nu anti-nu. It is shown that these purely long-distance contributions, arising from the exchange of a charged lepton, can be significant in B+ decays for an intermediate tau, potentially blurring the distinction between the modes used to extract B --> tau nu and those used to probe the genuine short-distance b --> (s,d) nu anti-nu FCNC transitions. Numerically, the tree-level contributions are found to account for 97%, 12% and 14% of the total B+ --> pi+ nu anti-nu, B+ --> K+ nu anti-nu, and B+ --> K*+ nu anti-nu rates, respectively.
description: 5 pages, 6 figures
MOESM19 of Deep sequencing on genome-wide scale reveals the unique composition and expression patterns of microRNAs in developing pollen of Oryza sativa
Creators: name: Wei, Li
name: Yan, Long
name: Wang, Tai
Publisher: name: figshare
Year: 2019
Subjects: subject: Medicine
subject: Genetics
subject: FOS: Biological sciences
subject: Molecular Biology
subject: Biological Sciences not elsewhere classified
subject: Information Systems not elsewhere classified
subject: Developmental Biology
subject: Plant Biology

description: Authorsâ original file for figure 6
The granularity of weakly occupied bosonic fields beyond the local density approximation
Creators: name: Eckart, M.
name: Walser, R.
name: Schleich, W. P.
name: Zöllner, S.
name: Schmelcher, P.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Other Condensed Matter (cond-mat.other)
subject: FOS: Physical sciences

description: We examine ground state correlations for repulsive, quasi one-dimensional bosons in a harmonic trap. In particular, we focus on the few particle limit N=2,3,4,..., where exact numerical solutions of the many particle Schroedinger equation are available employing the Multi-Configuration Time-dependent Hartree method. Our numerical results for the inhomogeneous system are modeled with the analytical solution of the homogeneous problem using the Bethe ansatz and the local density approximation. Tuning the interaction strength from the weakly correlated Gross-Pitaevskii- to the strongly correlated Tonks-Girardeau regime reveals finite particle number effects in the second order correlation function beyond the local density approximation.
description: 20 pages, 9 figures, submitted to NJP
Macroscopic Quantum Tunneling Effect of Z2 Topological Order
Creators: name: Yu, Jing
name: Kou, Su-Peng
Publisher: name: arXiv
Year: 2009
Subjects: subject: Strongly Correlated Electrons (cond-mat.str-el)
subject: FOS: Physical sciences

description: In this paper, macroscopic quantum tunneling (MQT) effect of Z2 topological order in the Wen-Plaquette model is studied. This kind of MQT is characterized by quantum tunneling processes of different virtual quasi-particles moving around a torus. By a high-order degenerate perturbation approach, the effective pseudo-spin models of the degenerate ground states are obtained. From these models, we get the energy splitting of the ground states, of which the results are consistent with those from exact diagonalization method
description: 25 pages, 14 figures, 4 tables
title: Ð¡Ð¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿ÑÐ¸Ñ Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸ Ð´ÐµÑÑÐºÐ¾Ð³Ð¾ ÑÑÐµÐ½ÐµÑÐ° Ð¿Ð¾ Ð»ÑÐ¶Ð½ÑÐ¼ Ð³Ð¾Ð½ÐºÐ°Ð¼ Ð¸ Ð±Ð¸Ð°ÑÐ»Ð¾Ð½Ñ
title: Social and psychological features of a childrenâs competitive skiing and biathlon coach
Creators: name: ÐÐ°Ð½Ð¶ÐµÐ»ÐµÐ¹, Ð.
name: ÐÑÑÐ°, Ð.
name: "Ð¡Ð¿Ð¾ÑÑ, ÑÐµÐ»Ð¾Ð²ÐµÐº, Ð·Ð´Ð¾ÑÐ¾Ð²ÑÐµ", Ð¼ÐµÐ¶Ð´ÑÐ½Ð°ÑÐ¾Ð´Ð½ÑÐ¹ Ð½Ð°ÑÑÐ½ÑÐ¹ ÐºÐ¾Ð½Ð³ÑÐµÑÑ
Publisher: name: ÐÐÐÐÐ¢ÐÐ¥-ÐÐ ÐÐ¡Ð¡
Year: 2021
Subjects: Ð´ÐµÑÑÐºÐ¸Ð¹ ÑÑÐµÐ½ÐµÑ
ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿ÑÐ¸Ñ Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÐ¸
ÑÑÑÐ´Ð½Ð¾ÑÑÐ¸
Ð·Ð½Ð°ÑÐ¸Ð¼ÑÐµ ÐºÐ°ÑÐµÑÑÐ²Ð°
ÑÐ´Ð¾Ð²Ð»ÐµÑÐ²Ð¾ÑÐµÐ½Ð½Ð¾ÑÑÑ

description: ÐÐ¾Ð»ÑÑÐµÐ½Ñ Ð½Ð¾Ð²ÑÐµ Ð´Ð°Ð½Ð½ÑÐµ Ð¾ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð¾ÑÐ¾Ð±ÐµÐ½Ð½Ð¾ÑÑÑÑ Ð´ÐµÑÑÐºÐ¸Ñ ÑÑÐµÐ½ÐµÑÐ¾Ð² (ÑÑÑÐ´Ð½Ð¾ÑÑÐ¸, ÐºÐ°ÑÑÐµÑÐ½ÑÐµ Ð¾ÑÐ¸ÐµÐ½ÑÐ°ÑÐ¸Ð¸, Ð·Ð½Ð°ÑÐ¸Ð¼ÑÐµ ÐºÐ°ÑÐµÑÑÐ²Ð°, ÑÐ´Ð¾Ð²Ð»ÐµÑÐ²Ð¾ÑÐµÐ½Ð½Ð¾ÑÑÑ), ÑÐµÐ°Ð»Ð¸Ð·ÑÑÑÐ¸Ñ Ð¿ÑÐ¾Ð³ÑÐ°Ð¼Ð¼Ñ ÑÐ¿Ð¾ÑÑÐ¸Ð²Ð½Ð¾Ð¹ Ð¿Ð¾Ð´Ð³Ð¾ÑÐ¾Ð²ÐºÐ¸ Ð¿Ð¾ Ð±Ð¸Ð°ÑÐ»Ð¾Ð½Ñ Ð¸ Ð»ÑÐ¶Ð½ÑÐ¼ Ð³Ð¾Ð½ÐºÐ°Ð¼, ÑÑÐ¾ Ð¿Ð¾Ð¼Ð¾Ð¶ÐµÑ Ð² ÑÐ¾ÑÐ¼Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸Ð¸ ÑÐµÐ³Ð¸Ð¾Ð½Ð°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¸ ÑÐµÐ´ÐµÑÐ°Ð»ÑÐ½Ð¾Ð³Ð¾ Ð¸Ð½ÑÐ¾ÑÐ¼Ð°ÑÐ¸Ð¾Ð½Ð½Ð¾Ð³Ð¾ Ð±Ð°Ð½ÐºÐ° Ð´Ð°Ð½Ð½ÑÑ Ð¾ ÑÐ¾ÑÐ¸Ð°Ð»ÑÐ½Ð¾-Ð¿ÑÐ¸ÑÐ¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ñ Ð´ÐµÑÐµÑÐ¼Ð¸Ð½Ð°Ð½ÑÐ°Ñ ÑÐ°Ð·Ð²Ð¸ÑÐ¸Ñ Ð´ÐµÑÑÐºÐ¾-ÑÐ½Ð¾ÑÐµÑÐºÐ¾Ð³Ð¾ ÑÐ¿Ð¾ÑÑÐ°.
description: The new data on the social and psychological characteristics of childrenâs coaches (difficulties, career orientations, significant qualities, satisfaction) who implement sports training programs in biathlon and cross-country skiing have been obtained. It will help in the formation of a regional and federal knowledge database on the social and psychological determinants for the development of children and youth sports.
Combined fit to BaBar and Belle Data on e+e- to phi pi+ pi- and phi f0(980)
Creators: name: Shen, C. P.
name: Yuan, C. Z.
Publisher: name: arXiv
Year: 2009
Subjects: subject: High Energy Physics - Experiment (hep-ex)
subject: FOS: Physical sciences

description: A combined fit is performed to the BaBar and Belle measurements of the $\EE \to ϕπ^+ π^-$ and $ϕ\fzero$ cross sections for center-of-mass energy between threshold and 3.0 GeV. The resonance parameters of the $ϕ(1680)$ and Y(2175) are determined. The mass is $(1681^{+10}_{-12})$ MeV/$c^2$ and the width is $(221^{+34}_{-24})$ MeV/$c^2$ for the $ϕ(1680)$, and the mass is $(2117^{+59}_{-49})$ MeV/$c^2$ and the width is $(164^{+69}_{-80})$ MeV/$c^2$ for the Y(2175). These information will shed light on the understanding of the nature of the excited $ϕ$ and $Y$ states observed in $\EE$ annihilation.
description: 10 pages, 6 figures
title: ÐÐ°Ð´Ð°ÑÐ¸, ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ñ Ð¸ ÑÐµÑÑÑ Ð¿Ð¾ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½Ðµ Â«ÐÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð¾ÑÐ»Ð¸Ð²Ð¾Ðº Ð¸Ð· ÑÐ¿Ð»Ð°Ð²Ð¾Ð² ÑÐ²ÐµÑÐ½ÑÑ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð²Â»
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: Ð¨ÐµÐ¼ÐµÑÐµÐ², ÐÑÐ¸Ð³Ð¾ÑÐ¸Ð¹
name: ÐÐ¾Ð±Ð¾Ñ, ÐÑÐ´Ð¼Ð¸Ð»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: Ð¦Ð²ÐµÑÐ½ÑÐµ Ð¼ÐµÑÐ°Ð»Ð»Ñ
Ð¡Ð¿Ð»Ð°Ð²Ñ
ÐÐ¸ÑÑÐµ Ñ ÑÐ´Ð¾Ð¶ÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ
ÐÐ»Ð°Ð²ÐºÐ° Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð²

description: Ð ÑÑÐµÐ±Ð½Ð¾Ð¼ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ð¸ Ð¿ÑÐ¸Ð²ÐµÐ´ÐµÐ½Ñ ÑÐµÑÑÑ Ð¸ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ñ, Ð½ÐµÐ¾Ð±ÑÐ¾Ð´Ð¸Ð¼ÑÐµ Ð¿ÑÐ¸ Ð¸Ð·ÑÑÐµÐ½Ð¸Ð¸ Ð´Ð¸ÑÑÐ¸Ð¿Ð»Ð¸Ð½ Â«ÐÑÐ¾Ð¸Ð·Ð²Ð¾Ð´ÑÑÐ²Ð¾ Ð¾ÑÐ»Ð¸Ð²Ð¾Ðº Ð¸Ð· ÑÐ²ÐµÑÐ½ÑÑ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð²Â», Â«Ð¦Ð²ÐµÑÐ½ÑÐµ Ð»Ð¸ÑÐµÐ¹Ð½ÑÐµ ÑÐ¿Ð»Ð°Ð²ÑÂ» Ð¸ Â«Ð¥ÑÐ´Ð¾Ð¶ÐµÑÑÐ²ÐµÐ½Ð½Ð¾Ðµ Ð»Ð¸ÑÑÐµÂ». Ð Ð¿ÐµÑÐ²Ð¾Ð¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ ÑÐ°ÑÑÐ¼Ð°ÑÑÐ¸Ð²Ð°ÐµÑÑÑ Ð²Ð»Ð¸ÑÐ½Ð¸Ðµ ÑÐ¾ÑÑÐ°Ð²Ð°, Ð¼Ð¾Ð´Ð¸ÑÐ¸ÑÐ¸ÑÐ¾Ð²Ð°Ð½Ð¸Ñ Ð¸ ÑÐºÐ¾ÑÐ¾ÑÑÐ¸ Ð¾ÑÐ»Ð°Ð¶Ð´ÐµÐ½Ð¸Ñ Ð½Ð° Ð¼ÐµÑÐ°Ð½Ð¸ÑÐµÑÐºÐ¸Ðµ Ð¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¸Ðµ ÑÐ²Ð¾Ð¹ÑÑÐ²Ð° Ð°Ð»ÑÐ¼Ð¸Ð½Ð¸ÐµÐ²ÑÑ, Ð¼Ð°Ð³Ð½Ð¸ÐµÐ²ÑÑ Ð¸ Ð¼ÐµÐ´Ð½ÑÑ ÑÐ¿Ð»Ð°Ð²Ð¾Ð². ÐÐ¾ Ð²ÑÐ¾ÑÐ¾Ð¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð¿ÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ ÑÐ¿ÑÐ°Ð¶Ð½ÐµÐ½Ð¸Ñ, ÑÐ²ÑÐ·Ð°Ð½Ð½ÑÐµ Ñ Ð¿ÑÐ¸Ð³Ð¾ÑÐ¾Ð²Ð»ÐµÐ½Ð¸ÐµÐ¼ ÑÐ°ÑÐ¿Ð»Ð°Ð²Ð° (Ð²Ð·Ð°Ð¸Ð¼Ð¾Ð´ÐµÐ¹ÑÑÐ²Ð¸ÐµÐ¼ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð² Ñ Ð³Ð°Ð·Ð°Ð¼Ð¸ Ð¸ ÑÐ°ÑÐ¸Ð½Ð¸ÑÐ¾Ð²Ð°Ð½Ð¸ÐµÐ¼ ÑÐ°ÑÐ¿Ð»Ð°Ð²Ð°). Ð ÑÑÐµÑÑÐµÐ¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð¿ÑÐ¸Ð²Ð¾Ð´Ð¸ÑÑÑ Ð°Ð»Ð³Ð¾ÑÐ¸ÑÐ¼ ÑÐ°Ð·ÑÐ°Ð±Ð¾ÑÐºÐ¸ ÑÐµÑÐ½Ð¾Ð»Ð¾Ð³Ð¸ÑÐµÑÐºÐ¾Ð³Ð¾ Ð¿ÑÐ¾ÑÐµÑÑÐ° Ð´Ð»Ñ ÑÐ¿Ð»Ð°Ð²Ð¾Ð² ÑÐ°Ð·Ð½Ð¾Ð³Ð¾ ÑÐ¾ÑÑÐ°Ð²Ð°. Ð ÑÐµÑÐ²ÐµÑÑÐ¾Ð¼ ÑÐ°Ð·Ð´ÐµÐ»Ðµ Ð¿ÑÐ¸Ð²Ð¾Ð´ÑÑÑÑ ÑÐµÑÑÑ Ð¿Ð¾ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐ¼ ÑÐ¿Ð¾ÑÐ¾Ð±Ð°Ð¼ Ð»Ð¸ÑÑÑ ÑÐ¿Ð»Ð°Ð²Ð¾Ð² ÑÐ²ÐµÑÐ½ÑÑ Ð¼ÐµÑÐ°Ð»Ð»Ð¾Ð² Ð¿Ð¾Ð´ Ð²Ð»Ð¸ÑÐ½Ð¸ÐµÐ¼ Ð²Ð½ÐµÑÐ½Ð¸Ñ Ð²Ð¾Ð·Ð´ÐµÐ¹ÑÑÐ²Ð¸Ð¹ (ÑÐ¿ÐµÑÐ¸Ð°Ð»ÑÐ½ÑÐµ ÑÐ¿Ð¾ÑÐ¾Ð±Ñ Ð»Ð¸ÑÑÑ).
Average Infrared Galaxy Spectra From Spitzer Flux Limited Samples
Creators: name: Weedman, Daniel W.
name: Houck, James R.
Publisher: name: arXiv
Year: 2008
Subjects: subject: Astrophysics (astro-ph)
subject: FOS: Physical sciences

description: The mid-infrared spectroscopic analysis of a flux-limited sample of galaxies with fv(24um) > 10 mJy is presented. Sources observed are taken from the Spitzer First Look Survey (FLS) catalog and from the NOAO Deep Wide-Field Survey region in Bootes (NDWFS). The spectroscopic sample includes 60 of the 100 sources in these combined catalogs having fv(24um) > 10 mJy. New spectra from the Spitzer Infrared Spectrograph are presented for 25 FLS sources and for 11 Bootes AGN; these are combined with 24 Bootes starburst galaxies previously published to determine the distribution of mid-infrared spectral characteristics for the total 10 mJy sample. Sources have 0.01 < z < 2.4 and 41.8 < log vLv(15um) < 46.2 (ergs/s). Average spectra are determined as a function of luminosity; lower luminosity sources (log vLv(15um) < 44.0) are dominated by PAH features and higher luminosity sources (log vLv(15um) > 44.0) are dominated by silicate absorption or emission. We find that a rest frame equivalent width of 0.4um for the 6.2um PAH emission feature provides a well defined division between lower luminosity, "pure" starbursts and higher luminosity AGN or composite sources. Using the average spectra, fluxes fv(24um) which would be observed with the Spitzer MIPS are predicted as a function of redshift for sources with luminosities that correspond to the average spectra. AGN identical to those in this 10 mJy sample could be seen to z = 3 with fv(24um) > 1 mJy, but starbursts fall to fv(24um) < 1 mJy by z ~ 0.5. This indicates that substantial luminosity evolution of starbursts is required to explain the numerous starbursts found in other IRS results having fv(24um) > 1 mJy and z ~ 2.
description: Accepted for publication in The Astrophysical Journal
Enlarging Holograms Under White Light, a Way to Save Holographic Material
Creators: name: Lunazzi, J. J.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Optics (physics.optics)
subject: FOS: Physical sciences

description: We developed techniques for employing holographic screens under white light, first exhibited to the public in 1989 (3) (4) which demonstrated the possibility of enlarging holograms already in 1990 (5). Fig. 1 shows how we encode views in a first step. The plane of the figure is horizontal, and a thin vertical slit is necessary to project each different view of the scene at a different sequential wavelength value. Decoding happens because the projected views are naturally angularly redistributed by the holographic screen (6).
description: 2 pages, 2 figures
I campioni italiani dell’astronomia
Creators: Daria Guidetti
Publisher: name: Media Inaf
Year: 2017

Giovedì 6 aprile si è svolta la cerimonia di premiazione con l’assegnazione della medaglia “Margherita Hack” alla rosa dei 10 vincitori della XV edizione delle Olimpiadi Italiane di Astronomia. Fra di loro, i 5 convocati per le finali internazionali
Le cronache del Sole
Creators: Francesca Aloisio
Publisher: name: Media Inaf
Year: 2017

Che l’arte e la letteratura siano fondamentali per la vita dell’uomo è fuor di dubbio, ma che lo fossero anche per la nostra comprensione dell'attività della nostra stella è una novità. Grazie ad una collaborazione tra la Kyoto University, il Japan's National Institute of Polar Research e il National Institute of Japanese Literature gli scienziati del Sol Levante sono riusciti a ricostruire la storia degli eventi solari del passato a partire dall’analisi di testi e documenti storici
Fuochi d’artificio stellari per Alma
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2017

Le antenne dell'Eso hanno ripreso una particolare fase violenta e scoppiettante che può caratterizzare la nascita di un gruppo particolarmente affollato di stelle. In questo caso, protagonista dell'immagine è la densa e attiva fabbrica stellare nota come OMC-1, nella costellazione di Orione
La migrazione violenta dei giganti caldi
Creators: Ufficio stampa Inaf
Publisher: name: Media Inaf
Year: 2017

Si chiamano gioviani caldi, e sono conosciuti anche come giganti gassosi o hot Jupiters: si tratta di una classe di esopianeti di cui abbiamo parlato spesso e sulla cui origine la nostra conoscenza fa oggi un importante passo avanti grazie al programma osservativo Gaps (Global Architecture of Planetary Systems). Due diversi studi a guida Inaf, infatti, uno coordinato da Aldo Bonomo, l’altro da Massimiliano Esposito, ci aiutano a comprendere meglio la loro formazione ed evoluzione
Hubble: un nuovo ritratto di Giove
Creators: Redazione Media Inaf
Publisher: name: Media Inaf
Year: 2017

Qualche giorno fa, Giove è arrivato vicino alla Terra e per vicino intendiamo quasi 668 milioni di chilometri. Il telescopio spaziale di Nasa ed Esa ha colto l'occasione per produrre un altro memorabile scatto del gigante gassoso
Rilevata atmosfera attorno a una simil-Terra
Creators: Stefano Parisini
Publisher: name: Media Inaf
Year: 2017

«Un primo passo verso lo studio delle atmosfere di pianeti di tipo terrestre», dice Luigi Mancini dell’Università di Roma Tor Vergata, tra gli scopritori di uno strato gassoso attorno a Gliese 1132b, che assurge al titolo di pianeta extrasolare con la gravità più simile alla Terra dotato di atmosfera
2MASS Two-Color Interstellar Reddening Lines: the Band-Width Effect
Creators: name: Straizys, V.
name: Lazauskaite, R.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: The band-width effect on interstellar reddening lines in the J-H vs. H-K_s diagram of the 2MASS survey is investigated using synthetic color indices and color excesses based on the Kurucz model atmospheres. At large interstellar reddenings (E(H-K_s) larger than 1.0) reddening lines deviate considerably from a straight line. The lines can be approximated by an equation: E(J-H) = r E(H-K_s) + s E(H-K_s)^2, where the slope coefficient, r, and the curvature coefficient, s, depend slightly on the intrinsic energy distribution of the source. The curvature of the reddening lines is confirmed by the J-H vs. H-K_s diagrams plotted by Straizys and Laugalys (2008) from 2MASS observations.
description: 6 pages, 1 figure
CCH in prestellar cores
Creators: name: Padovani, M.
name: Walmsley, C. M.
name: Tafalla, M.
name: Galli, D.
name: Müller, H. S. P.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We study the abundance of CCH in prestellar cores both because of its role in the chemistry and because it is a potential probe of the magnetic field. We also consider the non-LTE behaviour of the N=1-0 and N=2-1 transitions of CCH and improve current estimates of the spectroscopic constants of CCH. We used the IRAM 30m radiotelescope to map the N=1-0 and N=2-1 transitions of CCH towards the prestellar cores L1498 and CB246. Towards CB246, we also mapped the 1.3 mm dust emission, the J=1-0 transition of N2H+ and the J=2-1 transition of C18O. We used a Monte Carlo radiative transfer program to analyse the CCH observations of L1498. We derived the distribution of CCH column densities and compared with the H2 column densities inferred from dust emission. We find that while non-LTE intensity ratios of different components of the N=1-0 and N=2-1 lines are present, they are of minor importance and do not impede CCH column density determinations based upon LTE analysis. Moreover, the comparison of our Monte-Carlo calculations with observations suggest that the non-LTE deviations can be qualitatively understood. For L1498, our observations in conjunction with the Monte Carlo code imply a CCH depletion hole of radius 9 x 10^{16} cm similar to that found for other C-containing species. We briefly discuss the significance of the observed CCH abundance distribution. Finally, we used our observations to provide improved estimates for the rest frequencies of all six components of the CCH(1-0) line and seven components of CCH(2-1). Based on these results, we compute improved spectroscopic constants for CCH. We also give a brief discussion of the prospects for measuring magnetic field strengths using CCH.
description: 14 pages, 13 figures, to be published in Astronomy and Astrophysics
title: ÐÐ°Ð»Ð¾Ð³Ð¾Ð¾Ð±Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ»ÐµÐºÑÐµÐµÐ²Ð°, ÐÐ°Ñ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: 2021
Subjects: Ð½Ð°Ð»Ð¾Ð³Ð¸
Ð½Ð°Ð»Ð¾Ð³Ð¾Ð¾Ð±Ð»Ð¾Ð¶ÐµÐ½Ð¸Ðµ
Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²Ð¾Ðµ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð¾
ÑÑÐµÐ±Ð½Ð¸ÐºÐ¸ Ð¸ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ñ Ð´Ð»Ñ Ð²ÑÐ·Ð¾Ð²

description: Ð Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ Ð²ÐºÐ»ÑÑÐµÐ½Ñ Ð¾ÑÐ½Ð¾Ð²Ð½ÑÐµ ÑÐµÐ¾ÑÐµÑÐ¸ÑÐµÑÐºÐ¸Ðµ Ð¿Ð¾Ð»Ð¾Ð¶ÐµÐ½Ð¸Ñ ÑÐ¾Ð²ÑÐµÐ¼ÐµÐ½Ð½Ð¾Ð³Ð¾ Ð½Ð°Ð»Ð¾Ð³Ð¾Ð²Ð¾Ð³Ð¾ Ð·Ð°ÐºÐ¾Ð½Ð¾Ð´Ð°ÑÐµÐ»ÑÑÑÐ²Ð° Ð Ð¾ÑÑÐ¸Ð¸ Ð¸ ÐºÐ¾Ð½ÑÑÐ¾Ð»ÑÐ½ÑÐµ Ð²Ð¾Ð¿ÑÐ¾ÑÑ Ð´Ð»Ñ ÑÐ°Ð¼Ð¾Ð¾ÑÐµÐ½ÐºÐ¸ Ð·Ð½Ð°Ð½Ð¸Ð¹ Ð¾Ð±ÑÑÐ°ÑÑÐ¸Ð¼Ð¸ÑÑ.
Star Formation in Luminous HII regions in M33
Creators: name: Relano, Monica
name: Kennicutt, Robert C.
Publisher: name: arXiv
Year: 2009
Subjects: subject: Astrophysics of Galaxies (astro-ph.GA)
subject: FOS: Physical sciences

description: We present a multiwavelength (ultraviolet, infrared, optical and CO) study of a set of luminous HII regions in M33: NGC 604, NGC 595, NGC 592, NGC 588 and IC131. We study the emission distribution in the interiors of the HII regions to investigate the relation between the dust emission at 8 micron and 24 micron and the location of the massive stars and gas. We find that the 24 micron emission is closely related to the location of the ionized gas, while the 8 micron emission is more related to the boundaries of the molecular clouds consistently with its expected association with photodissociation regions (PDRs). Ultraviolet emission is generally surrounded by the H-alpha emission. For NGC 604 and NGC 595, where CO data are available, we see a radial gradient of the emission distribution at the wavelengths studied here: from the center to the boundary of the HII regions we observe ultraviolet, H-alpha, 24 micron, 8 micron and CO emission distributions. We quantify the star formation for our HII regions using the integrated fluxes at the set of available wavelengths, assuming an instantaneous burst of star formation. We show that a linear combination of 24 micron and H-alpha emission better describes the star formation for these objects than the dust luminosities by themselves. For NGC 604, we obtain and compare extinction maps derived from the Balmer decrement and from the 24 micron and H-alpha emission line ratio. Although the maps show locally different values in extinction, we find similar integrated extinctions derived from the two methods. We also investigate here the possible existence of embedded star formation within NGC 604.
description: 46 pages, 12 figures, accepted for publication in The Astrophysical Journal; pdf format available at http://www.ast.cam.ac.uk/~mrelano/
title: ÐÐµÑÐ°Ð»Ð»Ð¾ÑÐµÐ¶ÑÑÐ¸Ðµ ÑÑÐ°Ð½ÐºÐ¸. ÐÐ¸Ð½ÐµÐ¼Ð°ÑÐ¸ÐºÐ° Ð¸ Ð½Ð°Ð»Ð°Ð´ÐºÐ°
title: ÑÑÐµÐ±Ð½Ð¾Ðµ Ð¿Ð¾ÑÐ¾Ð±Ð¸Ðµ
titleType: Subtitle
Creators: name: ÐÐ¾Ð»ÑÐ²ÐºÐ¾, Ð.
name: ÐÐµÑÐµÐ»Ð¾Ð¼Ð¾Ð², Ð.
name: Ð¨Ð¼Ð°ÐºÐ¾Ð², Ð.
Publisher: name: ÐÐ·Ð´-Ð²Ð¾ Ð¡ÐÐ±ÐÐ¢Ð£
Year: 1998
Subjects: ÐÐµÑÐ°Ð»Ð»Ð¾ÑÐµÐ¶ÑÑÐ¸Ðµ ÑÑÐ°Ð½ÐºÐ¸

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