Galaxy-scale Star Formation on the Red Sequence: the Continued Growth of S0s and the Quiescence of Ellipticals
Samir Salim, Jerome J. Fang, R. Michael Rich, S. M. Faber, David A., Thilker

TL;DR
This study reveals that many S0 galaxies on the red sequence exhibit low-level, galaxy-scale star formation fueled by gas accretion, challenging the notion that all early-type galaxies are quiescent.
Contribution
It provides detailed high-resolution imaging evidence that S0 galaxies can sustain or resume star formation through gas accretion, distinguishing them from true ellipticals.
Findings
93% of studied ETGs show structured UV morphology indicating ongoing SF.
Galaxy-scale SF is mostly found in S0 galaxies, not ellipticals.
Star formation is fueled by gas accreted from the IGM or minor mergers.
Abstract
This paper examines star formation (SF) in relatively massive, primarily early-type galaxies (ETGs) at z~0.1. A sample is drawn from bulge-dominated GALEX/SDSS galaxies on the optical red sequence with strong UV excess and yet quiescent SDSS spectra. High-resolution far-UV imaging of 27 such ETGs using HST ACS/SBC reveals structured UV morphology in 93% of the sample, consistent with low-level ongoing SF (~0.5 Ms/yr). In 3/4 of the sample the SF is extended on galaxy scales (25-75 kpc), while the rest contains smaller (5-15 kpc) SF patches in the vicinity of an ETG - presumably gas-rich satellites being disrupted. Optical imaging reveals that all ETGs with galaxy-scale SF in our sample have old stellar disks (mostly S0 type). None is classified as a true elliptical. In our sample, galaxy-scale SF takes the form of UV rings of varying sizes and morphologies. For the majority of such…
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