Abundance determinations in extragalactic HII regions

The abundance determinations in extragalactic H װ regions are reviewed. The discussion is mainly focused on the different variants of the strong line method (calibrations). However, we do not list and consider in details a numerous relations suggested to convert metallicity-sensitive emission-line c...

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Збережено в:
Бібліографічні деталі
Дата:2013
Автор: Pilyugin, L.S.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2013
Назва видання:Advances in Astronomy and Space Physics
Онлайн доступ:http://dspace.nbuv.gov.ua/handle/123456789/119419
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Abundance determinations in extragalactic HII regions / L.S. Pilyugin // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 1. — С. 3-11. — Бібліогр.: 67 назв. — англ.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
id irk-123456789-119419
record_format dspace
spelling irk-123456789-1194192017-06-07T03:03:42Z Abundance determinations in extragalactic HII regions Pilyugin, L.S. The abundance determinations in extragalactic H װ regions are reviewed. The discussion is mainly focused on the different variants of the strong line method (calibrations). However, we do not list and consider in details a numerous relations suggested to convert metallicity-sensitive emission-line combinations into metallicity or temperature estimates. Instead we analyse the foundations of difierent types of calibrations and problems which those calibrations encounter. The empirical (defined by the H װ regions with well-measured abundances) and theoretical or model (defined by the set of photoionization models of H װ regions) metallicity scales are discussed. 2013 Article Abundance determinations in extragalactic HII regions / L.S. Pilyugin // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 1. — С. 3-11. — Бібліогр.: 67 назв. — англ. 2227-1481 http://dspace.nbuv.gov.ua/handle/123456789/119419 en Advances in Astronomy and Space Physics Головна астрономічна обсерваторія НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
description The abundance determinations in extragalactic H װ regions are reviewed. The discussion is mainly focused on the different variants of the strong line method (calibrations). However, we do not list and consider in details a numerous relations suggested to convert metallicity-sensitive emission-line combinations into metallicity or temperature estimates. Instead we analyse the foundations of difierent types of calibrations and problems which those calibrations encounter. The empirical (defined by the H װ regions with well-measured abundances) and theoretical or model (defined by the set of photoionization models of H װ regions) metallicity scales are discussed.
format Article
author Pilyugin, L.S.
spellingShingle Pilyugin, L.S.
Abundance determinations in extragalactic HII regions
Advances in Astronomy and Space Physics
author_facet Pilyugin, L.S.
author_sort Pilyugin, L.S.
title Abundance determinations in extragalactic HII regions
title_short Abundance determinations in extragalactic HII regions
title_full Abundance determinations in extragalactic HII regions
title_fullStr Abundance determinations in extragalactic HII regions
title_full_unstemmed Abundance determinations in extragalactic HII regions
title_sort abundance determinations in extragalactic hii regions
publisher Головна астрономічна обсерваторія НАН України
publishDate 2013
url http://dspace.nbuv.gov.ua/handle/123456789/119419
citation_txt Abundance determinations in extragalactic HII regions / L.S. Pilyugin // Advances in Astronomy and Space Physics. — 2013. — Т. 3., вип. 1. — С. 3-11. — Бібліогр.: 67 назв. — англ.
series Advances in Astronomy and Space Physics
work_keys_str_mv AT pilyuginls abundancedeterminationsinextragalactichiiregions
first_indexed 2023-10-18T20:34:31Z
last_indexed 2023-10-18T20:34:31Z
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