Hα star formation rates for a sample of star-forming galaxies from SDSS (DR1)

A study of current star formation rates (SFRs) derived from Hα emission of ionized hydrogen for 1305 star-forming galaxies from the Sloan Digital Sky Survey (Data Release 1) is carried out. Current SFRs are derived from the Hα flux corrected for interstellar extinction and aperture. For a subsample...

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Published in:Кинематика и физика небесных тел
Date:2005
Main Authors: Izotova, I.Y., Parnovsky, S.L., Izotov, Y.I.
Format: Article
Language:English
Published: Головна астрономічна обсерваторія НАН України 2005
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Online Access:https://nasplib.isofts.kiev.ua/handle/123456789/79654
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Journal Title:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Cite this:Hα star formation rates for a sample of star-forming galaxies from SDSS (DR1) / I.Y. Izotova, S.L. Parnovsky, Y.I. Izotov // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 262-265. — Бібліогр.: 13 назв. — англ.

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Digital Library of Periodicals of National Academy of Sciences of Ukraine
id nasplib_isofts_kiev_ua-123456789-79654
record_format dspace
spelling Izotova, I.Y.
Parnovsky, S.L.
Izotov, Y.I.
2015-04-03T17:38:12Z
2015-04-03T17:38:12Z
2005
Hα star formation rates for a sample of star-forming galaxies from SDSS (DR1) / I.Y. Izotova, S.L. Parnovsky, Y.I. Izotov // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 262-265. — Бібліогр.: 13 назв. — англ.
0233-7665
https://nasplib.isofts.kiev.ua/handle/123456789/79654
A study of current star formation rates (SFRs) derived from Hα emission of ionized hydrogen for 1305 star-forming galaxies from the Sloan Digital Sky Survey (Data Release 1) is carried out. Current SFRs are derived from the Hα flux corrected for interstellar extinction and aperture. For a subsample of 45 galaxies the current SFRs are derived using simultaneously three parameters: the galaxy luminosity in the far infrared range (IRAS data), the monochromatic radio continuum luminosity at 1.4 GHz (NVSS data), and the Hα emission of ionized hydrogen (SDSS DR1 data). The results obtained are discussed and compared with the similar ones for the Markarian galaxies.
en
Головна астрономічна обсерваторія НАН України
Кинематика и физика небесных тел
MS3: Physics of Stars and Galaxies
Hα star formation rates for a sample of star-forming galaxies from SDSS (DR1)
Article
published earlier
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
title Hα star formation rates for a sample of star-forming galaxies from SDSS (DR1)
spellingShingle Hα star formation rates for a sample of star-forming galaxies from SDSS (DR1)
Izotova, I.Y.
Parnovsky, S.L.
Izotov, Y.I.
MS3: Physics of Stars and Galaxies
title_short Hα star formation rates for a sample of star-forming galaxies from SDSS (DR1)
title_full Hα star formation rates for a sample of star-forming galaxies from SDSS (DR1)
title_fullStr Hα star formation rates for a sample of star-forming galaxies from SDSS (DR1)
title_full_unstemmed Hα star formation rates for a sample of star-forming galaxies from SDSS (DR1)
title_sort hα star formation rates for a sample of star-forming galaxies from sdss (dr1)
author Izotova, I.Y.
Parnovsky, S.L.
Izotov, Y.I.
author_facet Izotova, I.Y.
Parnovsky, S.L.
Izotov, Y.I.
topic MS3: Physics of Stars and Galaxies
topic_facet MS3: Physics of Stars and Galaxies
publishDate 2005
language English
container_title Кинематика и физика небесных тел
publisher Головна астрономічна обсерваторія НАН України
format Article
description A study of current star formation rates (SFRs) derived from Hα emission of ionized hydrogen for 1305 star-forming galaxies from the Sloan Digital Sky Survey (Data Release 1) is carried out. Current SFRs are derived from the Hα flux corrected for interstellar extinction and aperture. For a subsample of 45 galaxies the current SFRs are derived using simultaneously three parameters: the galaxy luminosity in the far infrared range (IRAS data), the monochromatic radio continuum luminosity at 1.4 GHz (NVSS data), and the Hα emission of ionized hydrogen (SDSS DR1 data). The results obtained are discussed and compared with the similar ones for the Markarian galaxies.
issn 0233-7665
url https://nasplib.isofts.kiev.ua/handle/123456789/79654
citation_txt Hα star formation rates for a sample of star-forming galaxies from SDSS (DR1) / I.Y. Izotova, S.L. Parnovsky, Y.I. Izotov // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 262-265. — Бібліогр.: 13 назв. — англ.
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first_indexed 2025-12-07T16:58:43Z
last_indexed 2025-12-07T16:58:43Z
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