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The GALEX Ultraviolet Atlas of Nearby Galaxies

Authors :
R. M. Rich
Young-Wook Lee
Tom A. Barlow
Patrick Morrissey
Sukyoung K. Yi
A. Boselli
Alexander S. Szalay
Susan G. Neff
Karl Forster
B. Milliard
Y. H. Joe
Luciana Bianchi
A. Gil de Paz
Tim Conrow
Samuel Boissier
Ted K. Wyder
Timothy M. Heckman
David Schiminovich
David A. Thilker
Mark Seibert
Peter G. Friedman
Jose Donas
Soo-Chang Rey
Barry F. Madore
D. C. Martin
Todd Small
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)
Beaussier, Catherine
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)
Source :
E-Prints Complutense. Archivo Institucional de la UCM, instname, E-Prints Complutense: Archivo Institucional de la UCM, Universidad Complutense de Madrid
Publication Year :
2006
Publisher :
HAL CCSD, 2006.

Abstract

We present images, integrated photometry, surface-brightness and color profiles for a total of 1034 nearby galaxies recently observed by the GALEX satellite in its far-ultraviolet (FUV; 1516A) and near-ultraviolet (NUV; 2267A) bands. (...) This data set has been complemented with archival optical, near-infrared, and far-infrared fluxes and colors. We find that the integrated (FUV-K) color provides robust discrimination between elliptical and spiral/irregular galaxies and also among spiral galaxies of different sub-types. Elliptical galaxies with brighter K-band luminosities (i.e. more massive) are redder in (NUV-K) color but bluer in (FUV-NUV) than less massive ellipticals. In the case of the spiral/irregular galaxies our analysis shows the presence of a relatively tight correlation between the (FUV-NUV) color and the total infrared-to-UV ratio. The correlation found between (FUV-NUV) color and K-band luminosity (with lower luminosity objects being bluer than more luminous ones) can be explained as due to an increase in the dust content with galaxy luminosity. The images in this Atlas along with the profiles and integrated properties are publicly available through a dedicated web page at http://nedwww.ipac.caltech.edu/level5/GALEX_Atlas/<br />Comment: 181 pages, 10 figures, accepted for publication in ApJS (abstract abridged)

Details

Language :
English
Database :
OpenAIRE
Journal :
E-Prints Complutense. Archivo Institucional de la UCM, instname, E-Prints Complutense: Archivo Institucional de la UCM, Universidad Complutense de Madrid
Accession number :
edsair.doi.dedup.....4fe64f5e24493954a90aa9a6cdb5cec7