UV emission and Star Formation in Stephan's Quintet
Abstract
we present the first GALEX UV images of the well known interacting group of galaxies, Stephan's Quintet (SQ). We detect widespread UV emission throughout the group. However, there is no consistent coincidence between UV structure and emission in the optical, H\alpha, or HI. Excluding the foreground galaxy NGC7320 (Sd), most of the UV emission is found in regions associated with the two spiral members of the group, NGC7319 and NGC7318b, and the intragroup medium starburst SQ-A. The extinction corrected UV data are analyzed to investigate the overall star formation activity in SQ. It is found that the total star formation rate (SFR) of SQ is 6.69+-0.65 M_\sun/yr. Among this, 1.34+-0.16 M_sun/yr is due to SQ-A. This is in excellent agreement with that derived from extinction corrected H\alpha luminosity of SQ-A. The SFR in regions related to NGC 7319 is 1.98+-0.58 M_\sun/yr, most of which(68%) is contributed by the disk. The contribution from the 'young tail' is only 15%. In the UV, the 'young tail' is more extended (~100 kpc) and shows a loop-like structure, including the optical tail, the extragalactic HII regions recently discovered in H\alpha, and other UV emission regions discovered for the first time. The UV and optical colors of the 'old tail' are consistent with a single stellar population of age t ~10^{8.5+-0.4} yrs. The UV emission associated with NGC 7318b is found in a very large (~80 kpc) disk, with a net SFR of 3.37+-0.25 M_sun/yr. Several large UV emission regions are 30 -- 40 kpc away from the nucleus of NGC7318b. Although both NGC7319 and NGC7318b show peculiar UV morphology, their SFR is consistent with that of normal Sbc galaxies, indicating that the strength of star formation activity is not enhenced by interactions.
Cite
@article{arxiv.astro-ph/0411319,
title = {UV emission and Star Formation in Stephan's Quintet},
author = {C. Kevin Xu and Jorge Iglesias-Paramo and Denis Burgarella and R. Michael Rich and Susan G. Neff and Sebastien Lauger and Tom A. Barlow and Luciana Bianchi and Yong-Ik Byun and Karl Forster and Peter G. Friedman and Timothy M. Heckman and Patrick N. Jelinsky and Young-Wook Lee and Barry F. Madore and Roger F. Malina and D. Christopher Martin and Bruno Milliard and Patrick Morrissey and David Schiminovich and Oswald H. W. Siegmund and Todd Small and Alex S. Szalay and Barry Y. Welsh and Ted K. Wyder},
journal= {arXiv preprint arXiv:astro-ph/0411319},
year = {2009}
}
Comments
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