Nitrogen abundance in the Blue Compact Dwarf galaxies from SDSS

We examined all of the galaxies in the Sloan Digital Sky Survey (SDSS) Data Release 7 (DR7) to select those with a dete ted [O ΙΙΙ ] λ4363 emission line, whih allows to derive electron temperatures in H װ regions and element abundan es by the diret method. We selected two sub-samples of galaxies: on...

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Бібліографічні деталі
Опубліковано в: :Advances in Astronomy and Space Physics
Дата:2015
Автор: Vovk, K.B.
Формат: Стаття
Мова:English
Опубліковано: Головна астрономічна обсерваторія НАН України 2015
Онлайн доступ:https://nasplib.isofts.kiev.ua/handle/123456789/119824
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Nitrogen abundance in the Blue Compact Dwarf galaxies from SDSS / K.B. Vovk // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 1. — С. 39-42. — Бібліогр.: 24 назв. — англ.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-119824
record_format dspace
spelling Vovk, K.B.
2017-06-09T21:02:22Z
2017-06-09T21:02:22Z
2015
Nitrogen abundance in the Blue Compact Dwarf galaxies from SDSS / K.B. Vovk // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 1. — С. 39-42. — Бібліогр.: 24 назв. — англ.
2227-1481
DOI: 10.17721/2227-1481.5.39-42
https://nasplib.isofts.kiev.ua/handle/123456789/119824
We examined all of the galaxies in the Sloan Digital Sky Survey (SDSS) Data Release 7 (DR7) to select those with a dete ted [O ΙΙΙ ] λ4363 emission line, whih allows to derive electron temperatures in H װ regions and element abundan es by the diret method. We selected two sub-samples of galaxies: one with detected WR features in their spectra, and the other with the nebular He װ λ4686 emission line. We confirm the increase of the N/O abundance ratio with decrease of the equivalent width EW(Hβ) of the Hβ emission line. This result is explained by gradual nitrogen enrihment of the interstellar medium by ejecta from massive stars in the most recent starburst episode.
en
Головна астрономічна обсерваторія НАН України
Advances in Astronomy and Space Physics
Nitrogen abundance in the Blue Compact Dwarf galaxies from SDSS
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Nitrogen abundance in the Blue Compact Dwarf galaxies from SDSS
spellingShingle Nitrogen abundance in the Blue Compact Dwarf galaxies from SDSS
Vovk, K.B.
title_short Nitrogen abundance in the Blue Compact Dwarf galaxies from SDSS
title_full Nitrogen abundance in the Blue Compact Dwarf galaxies from SDSS
title_fullStr Nitrogen abundance in the Blue Compact Dwarf galaxies from SDSS
title_full_unstemmed Nitrogen abundance in the Blue Compact Dwarf galaxies from SDSS
title_sort nitrogen abundance in the blue compact dwarf galaxies from sdss
author Vovk, K.B.
author_facet Vovk, K.B.
publishDate 2015
language English
container_title Advances in Astronomy and Space Physics
publisher Головна астрономічна обсерваторія НАН України
format Article
description We examined all of the galaxies in the Sloan Digital Sky Survey (SDSS) Data Release 7 (DR7) to select those with a dete ted [O ΙΙΙ ] λ4363 emission line, whih allows to derive electron temperatures in H װ regions and element abundan es by the diret method. We selected two sub-samples of galaxies: one with detected WR features in their spectra, and the other with the nebular He װ λ4686 emission line. We confirm the increase of the N/O abundance ratio with decrease of the equivalent width EW(Hβ) of the Hβ emission line. This result is explained by gradual nitrogen enrihment of the interstellar medium by ejecta from massive stars in the most recent starburst episode.
issn 2227-1481
url https://nasplib.isofts.kiev.ua/handle/123456789/119824
citation_txt Nitrogen abundance in the Blue Compact Dwarf galaxies from SDSS / K.B. Vovk // Advances in Astronomy and Space Physics. — 2015. — Т. 5., вип. 1. — С. 39-42. — Бібліогр.: 24 назв. — англ.
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last_indexed 2025-12-07T19:03:49Z
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