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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Опубліковано в: :Advances in Astronomy and Space Physics
Дата:2011
Автор: Shaldenkova, E.S.
Формат: Стаття
Мова:English
Опубліковано: Advances in astronomy and space physics 2011
Онлайн доступ:https://nasplib.isofts.kiev.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.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-118976
record_format dspace
spelling Shaldenkova, E.S.
2017-06-02T18:30:05Z
2017-06-02T18:30:05Z
2011
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
https://nasplib.isofts.kiev.ua/handle/123456789/118976
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.
I would like to thank my research supervisor Prof. A. V. Zasov. I also appreciate to authors for the possibility to use Hyperleda database.
en
Advances in astronomy and space physics
Advances in Astronomy and Space Physics
Atomic hydrogen deficiency in spiral galaxies in clusters
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Atomic hydrogen deficiency in spiral galaxies in clusters
spellingShingle Atomic hydrogen deficiency in spiral galaxies in clusters
Shaldenkova, E.S.
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
author Shaldenkova, E.S.
author_facet Shaldenkova, E.S.
publishDate 2011
language English
container_title Advances in Astronomy and Space Physics
publisher Advances in astronomy and space physics
format Article
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.
isbn 987-966-439-367-3
url https://nasplib.isofts.kiev.ua/handle/123456789/118976
fulltext
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.
work_keys_str_mv AT shaldenkovaes atomichydrogendeficiencyinspiralgalaxiesinclusters
first_indexed 2025-11-26T14:23:46Z
last_indexed 2025-11-26T14:23:46Z
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