The SAMI galaxy survey: A range in S0 properties indicating multiple formation pathways
It has been proposed that S0 galaxies are either fading spirals or the result of galaxy mergers. The relative contribution of each pathway and the environments in which they occur remain unknown. Here, we investigate stellar and gas kinematics of 219 S0s in the SAMI Survey to look for signs of multiple formation pathways occurring across the full range of environments. We identify a large range of rotational support in their stellar kinematics, which correspond to ranges in their physical...[Show more]
|ANU Research Publications
|Monthly Notices of the Royal Astronomical Society
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