The SLUGGS Survey: revisiting the correlation between X-ray luminosity and total mass of massive early-type galaxies
arXiv:1609.01713 · doi:10.1093/mnrasl/slw176
Abstract
Here we utilise recent measures of galaxy total dynamical mass and X-ray gas luminosities (L) for a sample of 29 massive early-type galaxies from the SLUGGS survey to probe L--mass scaling relations. In particular, we investigate scalings with stellar mass, dynamical mass within 5 effective radii (R) and total virial mass. We also compare these relations with predictions from CDM simulations. We find a strong linear relationship between L and galaxy dynamical mass within 5 R, which is consistent with the recent cosmological simulations of Choi et al. that incorporate mechanical heating from AGN. We conclude that the gas surrounding massive early-type galaxies was shock heated as it fell into collapsing dark matter halos so that L is primarily driven by the depth of a galaxy's potential well. Heating by an AGN plays an important secondary role in determining L.
arXiv comment5 pages, 2 figures, accepted for publication in MNRAS Letters
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