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Quenched fractions in the IllustrisTNG simulations: the roles of AGN feedback, environment, and pre-processing

2020/08/31 by Martina Donnari, Annalisa Pillepich, Gandhali D. Joshi +8 · 1 citation
Physics and Astronomy · #astro-ph.GA #astro-ph.CO

paper · pdf · doi:10.1093/mnras/staa3006

21 Pages, 11 figures, 2 tables, 1 appendix, published in MNRAS

arxiv created 2020/10/14 · arxiv updated 2020/10/15

Abstract

We use the IllustrisTNG simulations to show how the fractions of quenched galaxies vary across different environments and cosmic time, and to quantify the role AGN feedback and preprocessing play in quenching group and cluster satellites. At z=0, we select galaxies with M_* = 109-12 M\odot residing within (≤ R200c) groups and clusters of total host mass M200c=1013-15.2 M\odot. TNG predicts a quenched fraction of ∼70-90% (on average) for centrals and satellites \gtrsim 1010.5 M\odot, regardless of host mass, cosmic time (0≤ z≤0.5), clustercentric distance and time since infall in the z=0 host. Low-mass centrals (\lesssim 1010 M\odot), instead, are rarely quenched unless they become members of groups (1013-14 M\odot) or clusters (≥1014 M\odot), where the quenched fraction rises to ∼80%. The fraction of low-mass passive galaxies is higher closer to the host center and for more massive hosts. The population of low-mass satellites accreted \gtrsim4-6 Gyr ago in massive hosts is almost entirely passive, thus suggesting an upper limit for the time needed for environmental quenching to occur. In fact, ∼30% of group and cluster satellites that are quenched at z=0 were already quenched before falling into their current host, and the bulk of them quenched as early as 4 to 10 billion years ago. For low-mass galaxies (\lesssim1010-10.5M\odot), this is due to preprocessing, whereby current satellites may have been members of other hosts, and hence have undergone environmental processes, before falling into their final host, this mechanism being more common and more effective for the purposes of quenching for satellites found today in more massive hosts. On the other hand, massive galaxies quench on their own and because of AGN feedback, regardless of whether they are centrals or satellites.

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