GeminiFocus 2014 Year in Review | Page 8

Figure 2. Top Panel: The average spectra of star-forming (blue) and poststarburst galaxies (green) in the GCLASS clusters. The black lines are the best-fit spectra for both types based on the star-formation history in the lowerleft panel. Lower-left panel: The best-fit star-formation history of the post-starburst galaxies under the assumption that the star-forming galaxies are their progenitors. This suggests that the average poststarburst spends ~ 2.3 Gyr forming stars before it is quenched on a timescale of ~ 0.1 ± 0.4 Gyr. This is fully consistent with the quenching model derived from dynamics of the galaxy populations in Figure 1. Towards a Physical Model of Satellite Quenching The overall picture that emerges from this analysis is that when star-forming galaxies fall into clusters they continue forming stars for 0.5 - 1.5 Gyr — about the time it takes to fall far enough into the cluster to cross about half of the virial radius. Once this happens, the quenching process begins, and it is quite rapid, perhaps even violent. Despite having concrete numbers to work with, there are still challenges in understanding exactly what is happening. For instance, because the quenching process appears to be so rapid, it’s tempting to believe that all gas — both hot and cold — is being removed from the galaxy. But that may not 6 GeminiFocus be the full story. Galaxies at z ~ 1 are forming stars at a much higher rate than those at z ~ 0. If only the hot gas was removed, the higher-redshift galaxies would consume most of their cold gas quite quickly, on a timescale of ~ 0.5 Gyr, which is the upper limit of what the models permit. So, there is clearly still work to do. Since we know that the cold gas consumption time-scales move to longer values at lower redshift, measuring any evolution in the quenching timescale with redshift is crucial for breaking this degeneracy. Some studies have been done at lower-redshift, and they tend to indicate slightly longer timescales than we measured at z ~ 1 (e.g., Wetzel et al., 2013; Haines et al., 2013). This would implicate hot gas stripping, but the analysis was 2014 Year in Review January 2015