Radial Distribution of Near-UV Flux in Disc Galaxies in the range 0<z<1

Details Radial Distribution of Near-UV Flux in Disc Galaxies in the range 0<z<1 Radial Distribution of Near-UV Flux in Disc Galaxies in the range 0<z<1

2009-03-24

arxiv.org/abs/0903.4140v1

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

26 pages, 21 figures, accepted for publication in Astronomy & Astrophysics on March 21st

Scientific paper

(Abridged) The goal of this paper is to quantify the changes on the SF distribution within the disc galaxies in the last ~8 Gyr. We use as a proxy for the SF radial profile the Near-UV surface brightness distributions, allowing suitably for extinction. We compare the effective radii (R_eff) and concentration of the flux distribution in the rest-frame Near-UV for a sample of 270 galaxies in the range 0

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