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Recent star formation in nearby galaxies from GALEX imaging:M101 and M51

Authors :
Bianchi, Luciana
Thilker, D.
Burgarella, D.
Friedman, P.
Hoopes, C.
Boissier, S.
de Paz, A. Gil
Barlow, T.
Byun, Y. -I.
Donas, J.
Forster, K.
Heckman, T.
Jelinsky, P.
Lee, Y-W
Madore, B.
Malina, R.
Martin, C.
Milliard, B.
Morrissey, P.
Neff, S.
Rich, M.
Schiminovich, D.
Siegmund, O.
Small, T.
Szalay, A.
Welsh, B.
Wyder, T.
Department of Physics and Astronomy [Baltimore]
Johns Hopkins University (JHU)
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)
Observatories [Carnegie Institution]
Carnegie Institution for Science [Washington]
Center for Space Astrophysics [Seoul]
Yonsei University
Space Sciences Laboratory [Berkeley] (SSL)
University of California [Berkeley]
University of California-University of California
Department of Physics and Astronomy [UCLA Los Angeles]
University of California [Los Angeles] (UCLA)
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)
Carnegie Institution for Science
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, 619, pp.L71-L74, The Astrophysical journal letters, 2005, 619, pp.L71-L74
Publication Year :
2005
Publisher :
HAL CCSD, 2005.

Abstract

The GALEX (Galaxy Evolution Explorer) Nearby Galaxies Survey is providing deep far-UV and near-UV imaging for a representative sample of galaxies in the local universe. We present early results for M51 and M101, from GALEX UV imaging and SDSS optical data in five bands. The multi-band photometry of compact stellar complexes in M101 is compared to population synthesis models, to derive ages, reddening, reddening-corrected luminosities and current/initial masses. The GALEX UV photometry provides a complete census of young compact complexes on a approximately 160pc scale. A galactocentric gradient of the far-UV - near-UV color indicates younger stellar populations towards the outer parts of the galaxy disks, the effect being more pronounced in M101 than in M51.<br />Comment: This paper will be published as part of the Galaxy Evolution Explorer (GALEX) Astrophysical Journal Letters Special Issue. Full paper available from http://dolomiti.pha.jhu.edu . Links to full set of papers will be available at http://www.galex.caltech.edu/PUBLICATIONS/ after November 22, 2004

Details

Language :
English
ISSN :
20418205 and 20418213
Database :
OpenAIRE
Journal :
The Astrophysical journal letters, The Astrophysical journal letters, Bristol : IOP Publishing, 2005, 619, pp.L71-L74, The Astrophysical journal letters, 2005, 619, pp.L71-L74
Accession number :
edsair.doi.dedup.....ef5c512e63a89abbd45774ce5006778a