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Extinction radial profiles of M83 from GALEX UV imaging

Authors :
Boissier, Samuel
de Paz, Armando Gil
Madore, B. F.
Boselli, A.
Buat, V.
Burgarella, D.
Friedman, P. G.
Barlow, T. A.
Bianchi, L.
Byun, Y. -I.
Donas, José
Forster, K.
Heckman, T. M.
Jelinsky, P. N.
Lee, Y. -W.
Malina, R. F.
Martin, D. C.
Milliard, B.
Morrissey, P.
Neff, Susan Gale
Rich, Robert Michael
Schiminovich, David
Siegmund, O. H. W.
Small, Todd
Szalay, Alex
Wyder, Ted
Welsh, B.
Institut d'Astrophysique de Paris (IAP)
Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)
Observatories [Carnegie Institution]
Carnegie Institution for Science [Washington]
Laboratoire d'Astrophysique de Marseille (LAM)
Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES)
California Institute of Technology (CALTECH)
Center for Astrophysical Sciences [Baltimore]
Johns Hopkins University (JHU)
Center for Space Astrophysics [Seoul]
Yonsei University
Department of Physics and Astronomy [Baltimore]
Space Sciences Laboratory [Berkeley] (SSL)
University of California [Berkeley]
University of California-University of California
Laboratory for Astronomy and Solar Physics
NASA Goddard Space Flight Center (GSFC)
Department of Physics and Astronomy [UCLA Los Angeles]
University of California [Los Angeles] (UCLA)
Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National de la Recherche Scientifique (CNRS)
Carnegie Institution for Science
Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
University of California [Berkeley] (UC Berkeley)
University of California (UC)-University of California (UC)
Source :
The Astrophysical journal letters, The Astrophysical journal letters, Bristol : IOP Publishing, 2005, 619L, pp.83B. ⟨10.1086/423668⟩, The Astrophysical journal letters, 2005, 619L, pp.83B. ⟨10.1086/423668⟩
Publication Year :
2005
Publisher :
HAL CCSD, 2005.

Abstract

We use the far-UV (FUV) and near-UV (NUV) images of M83 obtained by GALEX to compute the radial profile of the UV spectral slope in the star forming disk. We briefly present a model of its chemical evolution which allows us to obtain realistic intrinsic properties of the stellar populations. Using corollary data, we also compute the profiles of H-alpha/H-beta and of the total IR (TIR) to FUV ratio. Both data and model are used to estimate and compare the extinction gradients at the FUV wavelength obtained from these various indicators. We discuss the implications for the determination of the star formation rate.<br />Comment: This paper will be published as part of the Galaxy Evolution Explorer (GALEX) Astrophysical Journal Letters Special Issue. Links to the full set of papers will be available at http://www.galex.caltech.edu/PUBLICATIONS/ after November 22, 2004. A high resolution version of figure 1 is available at http://www.ociw.edu/~boissier/M83/fig1.ps

Details

Language :
English
ISSN :
20418205 and 20418213
Database :
OpenAIRE
Journal :
The Astrophysical journal letters, The Astrophysical journal letters, Bristol : IOP Publishing, 2005, 619L, pp.83B. ⟨10.1086/423668⟩, The Astrophysical journal letters, 2005, 619L, pp.83B. ⟨10.1086/423668⟩
Accession number :
edsair.doi.dedup.....d567debcf9c545b55a98b2f8f29cf4fc
Full Text :
https://doi.org/10.1086/423668⟩