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 |
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| Date: | 2005 |
| Main Authors: | , , |
| Format: | Article |
| Language: | English |
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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 |
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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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1850869518956494848 |