SIMBAD references

2014ApJ...792..141S - Astrophys. J., 792, 141 (2014/September-2)

The mass dependence of dwarf satellite galaxy quenching.

SLATER C.T. and BELL E.F.

Abstract (from CDS):

We combine observations of the Local Group with data from the NASA-Sloan Atlas to show the variation in the quenched fraction of satellite galaxies from low-mass dwarf spheroidals and dwarf irregulars to more massive dwarfs similar to the Magellanic Clouds. While almost all of the low-mass (M{sstarf} ≲ 107 M) dwarfs are quenched, at higher masses the quenched fraction decreases to approximately 40%-50%. This change in the quenched fraction is large and suggests a sudden change in the effectiveness of quenching that correlates with satellite mass. We combine this observation with models of satellite infall and ram pressure stripping to show that the low-mass satellites must quench within 1-2 Gyr of pericenter passage to maintain a high quenched fraction, but that many more massive dwarfs must continue to form stars today even though they likely fell into their host >5 Gyr ago. We also characterize how the susceptibility of dwarfs to ram pressure must vary as a function of mass if it is to account for the change in quenched fractions. Though neither model predicts the quenching effectiveness a priori, this modeling illustrates the physical requirements that the observed quenched fractions place on possible quenching mechanisms.

Abstract Copyright:

Journal keyword(s): galaxies: dwarf - galaxies: evolution - Local Group

Simbad objects: 9

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2019.10.14-14:31:46

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