Cambridge University Press (CUP), Proceedings of the International Astronomical Union, H16(10), p. 132-132, 2012
DOI: 10.1017/s1743921314004931
Full text: Unavailable
AbstractWe measured the UV-optical-near-IR spectral energy distributions (SEDs) of redshift z ~ 0.3-1.5 early-type galaxies (ETGs) with the Hubble Space Telescope (HST) Wide Field Camera 3 (Rutkowski et al.2012). We searched for young stellar populations and morphological signatures of the mechanisms driving recent star formation (RSF) in these ETGs in order to provide observational constraints on models of galaxy evolution.