Permanent URL to this publication: http://dx.doi.org/10.5167/uzh-60039
Just, D W; Zaritsky, D; Tran, K V H; Gonzalez, A H; Kautsch, S J; Moustakas, J (2011). A search for young stars in the S0 galaxies of a super-group at z=0.37. Astrophysical Journal, 740(2):54.
|Published Version (English)|
PDF - Registered users only
We analyze GALEX UV data for a system of four gravitationally-bound groups at z=0.37, SG1120, which is destined to merge into a Coma-mass cluster by z=0, to study how galaxy properties may change during cluster assembly. Of the 38 visually-classified S0 galaxies, with masses ranging from log(M_*)~10-11, we detect only one in the NUV channel, a strongly star-forming S0 that is the brightest UV source with a measured redshift placing it in SG1120. Stacking the undetected S0 galaxies (which generally lie on or near the optical red-sequence of SG1120) still results in no NUV/FUV detection (<2 sigma). Using our limit in the NUV band, we conclude that for a rapidly truncating star formation rate, star formation ceased *at least* ~0.1 to 0.7 Gyr ago, depending on the strength of the starburst prior to truncation. With an exponentially declining star-formation history over a range of time-scales, we rule out recent star-formation over a wide range of ages. We conclude that if S0 formation involves significant star formation, it occurred well before the groups were in this current pre-assembly phase. As such, it seems that S0 formation is even more likely to be predominantly occurring outside of the cluster environment.
|Item Type:||Journal Article, refereed, original work|
|Communities & Collections:||07 Faculty of Science > Institute for Computational Science|
|Deposited On:||23 Feb 2012 21:36|
|Last Modified:||19 Jun 2014 20:51|
|Publisher:||Institute of Physics Publishing|
|Citations:||Web of Science®. Times Cited: 5|
Scopus®. Citation Count: 3
Users (please log in): suggest update or correction for this item
Repository Staff Only: item control page