{ "id": "1409.6683", "version": "v1", "published": "2014-09-23T17:58:33.000Z", "updated": "2014-09-23T17:58:33.000Z", "title": "Early-type galaxies at intermediate redshift observed with HST WFC3: perspectives on recent star-formation", "authors": [ "M. Rutkowski", "H. Jeong", "S. H. Cohen", "S. Kaviraj", "R. E. Ryan, Jr.", "R. A. Windhorst", "A. Koekemoer", "N. P. Hathi", "M. A. Dopita", "S. K. Yi" ], "comment": "Accepted for publication in ApJ", "categories": [ "astro-ph.GA" ], "abstract": "We present an analysis of the stellar populations of 102 visually-selected early-type galaxies (ETGs) with spectroscopic redshifts (0.310.5) recently star-forming ETGs appear to have larger sizes. Furthermore, high-mass, quiescent ETGs identified with likely companions populate a distinct region in the size-mass parameter space, in comparison with the distribution of massive ETGs with evidence of RSF. We conclude that both mechanisms of the quenching of star-formation in disk-like ETGs and (gas-rich, minor) merger activity contribute to the formation of young stars and the size-mass evolution of intermediate redshift ETGs. The number of ETGs for which we have both HST WFC3 panchromatic (especially UV) imaging and spectroscopically-confirmed redshifts is relatively small, therefore a conclusion on the relative roles of both of these mechanisms remains an open question.", "revisions": [ { "version": "v1", "updated": "2014-09-23T17:58:33.000Z" } ], "analyses": { "keywords": [ "star-formation", "perspectives", "intermediate redshift etgs", "merger activity contribute", "hst wfc3 panchromatic" ], "publication": { "doi": "10.1088/0004-637X/796/2/101", "journal": "The Astrophysical Journal", "year": 2014, "month": "Dec", "volume": 796, "number": 2, "pages": 101 }, "note": { "typesetting": "TeX", "pages": 0, "language": "en", "license": "arXiv", "status": "editable", "adsabs": "2014ApJ...796..101R" } } }