most citedThe Look-back Time Evolution of Far-Ultraviolet Flux from the Brightest Cluster Elliptical Galaxies at z < 0.2

46 citations · 50 across the 2 of their papers we have counts for

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astro-ph20074 cited

The Curious Case of NGC6908

B. F. Madore, A. Gil de Paz, O. Pevunova +1

The object NGC6908 was once thought to be simply a surface-brightness enhancement in the eastern spiral arm of the nearby spiral galaxy NGC6907. Based on an examination of near-inf…

astro-ph200746 cited

The Look-back Time Evolution of Far-Ultraviolet Flux from the Brightest Cluster Elliptical Galaxies at z < 0.2

Chang H. Ree, Young-Wook Lee, Sukyoung K. Yi +28

We present the GALEX UV photometry of the elliptical galaxies in Abell clusters at moderate redshifts (z < 0.2) for the study of the look-back time evolution of the UV upturn pheno…

astro-ph2004

Extinction radial profiles of M83 from GALEX UV imaging

S. Boissier, A. Gil de Paz, B. F. Madore +24

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 mode…

astro-ph2004

New Constraints on the Star Formation Histories and Dust Attenuation of Galaxies in the Local Universe from GALEX

Samir Salim, Stephane Charlot, R. Michael Rich +23

We derive a variety of physical parameters including star formation rates (SFRs), dust attenuation and burst mass fractions for 6472 galaxies observed by the Galaxy Evolution Explo…

astro-ph2004

UV Morphology and Star Formation in the Tidal Tails of NGC 4038/39

J. E. Hibbard, L. Bianchi, D. A. Thilker +2

We present GALEX FUV (1530 A) and NUV (2310 A) observations of the archetypal merging system NGC 4038/39, ``The Antennae". Both tails are relatively bright in the UV, especially in…

astro-ph2004

GALEX Observations of the Ultraviolet Halos of NGC 253 and M82

C. G. Hoopes, T. M. Heckman, D. K. Strickland +25

We present Galaxy Evolution Explorer (GALEX) images of the prototypical edge-on starburst galaxies M82 and NGC253. Our initial analysis is restricted to the complex of ultraviolet…