Attenuation Laws for Galaxies with Different Star Formation Histories, Based on the SDSS Images
Attenuation curves (laws) in the optical part of thespectrum (from about 3500 AA~to 9000 AA) are determined for galaxieswith different star formation histories (SFHs) using images in five photometrical bands from the Sloan Digital Sky Survey (SDSS). Owing to large surveys like SDSS, it is possible t...
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Astronomical Observatory, Department of Astronomy, Belgrade
2009-06-01
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doaj-4996c570515e47769bea36b359e911822020-11-25T02:24:45ZengAstronomical Observatory, Department of Astronomy, BelgradeSerbian Astronomical Journal1450-698X2009-06-011782127Attenuation Laws for Galaxies with Different Star Formation Histories, Based on the SDSS ImagesVince, O.Attenuation curves (laws) in the optical part of thespectrum (from about 3500 AA~to 9000 AA) are determined for galaxieswith different star formation histories (SFHs) using images in five photometrical bands from the Sloan Digital Sky Survey (SDSS). Owing to large surveys like SDSS, it is possible to defineseveral subgroups of galaxies with similar SFHs using two spectralindices that trace SFH. Attenuation curves are analyzed in termsof SFH and compared to the curves that are often used for dustcorrection of the observed data.http://saj.matf.bg.ac.rs/178/pdf/021-027.pdfGalaxies: photometryGalaxies: ISMGalaxies: stellar content |
collection |
DOAJ |
language |
English |
format |
Article |
sources |
DOAJ |
author |
Vince, O. |
spellingShingle |
Vince, O. Attenuation Laws for Galaxies with Different Star Formation Histories, Based on the SDSS Images Serbian Astronomical Journal Galaxies: photometry Galaxies: ISM Galaxies: stellar content |
author_facet |
Vince, O. |
author_sort |
Vince, O. |
title |
Attenuation Laws for Galaxies with Different Star Formation Histories, Based on the SDSS Images |
title_short |
Attenuation Laws for Galaxies with Different Star Formation Histories, Based on the SDSS Images |
title_full |
Attenuation Laws for Galaxies with Different Star Formation Histories, Based on the SDSS Images |
title_fullStr |
Attenuation Laws for Galaxies with Different Star Formation Histories, Based on the SDSS Images |
title_full_unstemmed |
Attenuation Laws for Galaxies with Different Star Formation Histories, Based on the SDSS Images |
title_sort |
attenuation laws for galaxies with different star formation histories, based on the sdss images |
publisher |
Astronomical Observatory, Department of Astronomy, Belgrade |
series |
Serbian Astronomical Journal |
issn |
1450-698X |
publishDate |
2009-06-01 |
description |
Attenuation curves (laws) in the optical part of thespectrum (from about 3500 AA~to 9000 AA) are determined for galaxieswith different star formation histories (SFHs) using images in five photometrical bands from the Sloan Digital Sky Survey (SDSS). Owing to large surveys like SDSS, it is possible to defineseveral subgroups of galaxies with similar SFHs using two spectralindices that trace SFH. Attenuation curves are analyzed in termsof SFH and compared to the curves that are often used for dustcorrection of the observed data. |
topic |
Galaxies: photometry Galaxies: ISM Galaxies: stellar content |
url |
http://saj.matf.bg.ac.rs/178/pdf/021-027.pdf |
work_keys_str_mv |
AT vinceo attenuationlawsforgalaxieswithdifferentstarformationhistoriesbasedonthesdssimages |
_version_ |
1724853523090243584 |