Atomic hydrogen deficiency in spiral galaxies in clusters

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 diamet...

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Дата:2011
Автор: Shaldenkova, E.S.
Формат: Стаття
Мова:English
Опубліковано: Advances in astronomy and space physics 2011
Назва видання:Advances in Astronomy and Space Physics
Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/118976
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати: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.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id irk-123456789-118976
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spelling irk-123456789-1189762017-06-03T03:02:43Z Atomic hydrogen deficiency in spiral galaxies in clusters Shaldenkova, E.S. 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. 2011 Article 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. 987-966-439-367-3 http://dspace.nbuv.gov.ua/handle/123456789/118976 en Advances in Astronomy and Space Physics Advances in astronomy and space physics
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
description 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.
format Article
author Shaldenkova, E.S.
spellingShingle Shaldenkova, E.S.
Atomic hydrogen deficiency in spiral galaxies in clusters
Advances in Astronomy and Space Physics
author_facet Shaldenkova, E.S.
author_sort Shaldenkova, E.S.
title Atomic hydrogen deficiency in spiral galaxies in clusters
title_short Atomic hydrogen deficiency in spiral galaxies in clusters
title_full Atomic hydrogen deficiency in spiral galaxies in clusters
title_fullStr Atomic hydrogen deficiency in spiral galaxies in clusters
title_full_unstemmed Atomic hydrogen deficiency in spiral galaxies in clusters
title_sort atomic hydrogen deficiency in spiral galaxies in clusters
publisher Advances in astronomy and space physics
publishDate 2011
url http://dspace.nbuv.gov.ua/handle/123456789/118976
citation_txt 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.
series Advances in Astronomy and Space Physics
work_keys_str_mv AT shaldenkovaes atomichydrogendeficiencyinspiralgalaxiesinclusters
first_indexed 2023-10-18T20:33:27Z
last_indexed 2023-10-18T20:33:27Z
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