Atomic hydrogen deficiency in spiral galaxies in clusters

dc.contributor.author	Shaldenkova, E.S.
dc.date.accessioned	2017-06-02T18:30:05Z
dc.date.available	2017-06-02T18:30:05Z
dc.date.issued	2011
dc.description.abstract	We consider the new method for atomic hydrogen deficiency estimations. The main idea is to use the empirical relation between total HI mass and specific angular momentum of the disk for isolated galaxies. The method was compared with the standard one, based on dependence of HI mass on optical diameter and galaxy type. They both were applied to Virgo and Coma cluster galaxies and to Local Volume galaxies. Also we investigated possible mechanisms responsible for HI deficiency in cluster spirals.	uk_UA
dc.description.sponsorship	I would like to thank my research supervisor Prof. A. V. Zasov. I also appreciate to authors for the possibility to use Hyperleda database.	uk_UA
dc.identifier.citation	Atomic hydrogen deficiency in spiral galaxies in clusters / E.S. Shaldenkova // Advances in Astronomy and Space Physics. — 2011. — Т. 1., вип. 1-2. — С. 23-26. — Бібліогр.: 25 назв. — англ.	uk_UA
dc.identifier.isbn	987-966-439-367-3
dc.identifier.uri	https://nasplib.isofts.kiev.ua/handle/123456789/118976
dc.language.iso	en	uk_UA
dc.publisher	Advances in astronomy and space physics	uk_UA
dc.relation.ispartof	Advances in Astronomy and Space Physics
dc.status	published earlier	uk_UA
dc.title	Atomic hydrogen deficiency in spiral galaxies in clusters	uk_UA
dc.type	Article	uk_UA

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