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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Veröffentlicht in:Advances in Astronomy and Space Physics
Datum:2013
1. Verfasser: Pilyugin, L.S.
Format: Artikel
Sprache:English
Veröffentlicht: Головна астрономічна обсерваторія НАН України 2013
Online Zugang:https://nasplib.isofts.kiev.ua/handle/123456789/119419
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Zitieren: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.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-119419
record_format dspace
spelling Pilyugin, L.S.
2017-06-06T19:05:19Z
2017-06-06T19:05:19Z
2013
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
https://nasplib.isofts.kiev.ua/handle/123456789/119419
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.
en
Головна астрономічна обсерваторія НАН України
Advances in Astronomy and Space Physics
Abundance determinations in extragalactic HII regions
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Abundance determinations in extragalactic HII regions
spellingShingle Abundance determinations in extragalactic HII regions
Pilyugin, L.S.
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
author Pilyugin, L.S.
author_facet Pilyugin, L.S.
publishDate 2013
language English
container_title Advances in Astronomy and Space Physics
publisher Головна астрономічна обсерваторія НАН України
format Article
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.
issn 2227-1481
url https://nasplib.isofts.kiev.ua/handle/123456789/119419
fulltext
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.
work_keys_str_mv AT pilyuginls abundancedeterminationsinextragalactichiiregions
first_indexed 2025-11-26T14:24:13Z
last_indexed 2025-11-26T14:24:13Z
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