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OBSERVING THE END OF COLD FLOW ACCRETION USING...
Journal article

OBSERVING THE END OF COLD FLOW ACCRETION USING HALO ABSORPTION SYSTEMS

Abstract

We use cosmological smoothed particle hydrodynamic simulations to study the cool, accreted gas in two Milky Way size galaxies through cosmic time to z = 0. We find that gas from mergers and cold flow accretion results in significant amounts of cool gas in galaxy halos. This cool circum-galactic component drops precipitously once the galaxies cross the critical mass to form stable shocks, Mvir = Msh ∼ 1012 M☉. Before reaching Msh, the galaxies …

Authors

Stewart KR; Kaufmann T; Bullock JS; Barton EJ; Maller AH; Diemand J; Wadsley J

Journal

The Astrophysical Journal Letters, Vol. 735, No. 1,

Publisher

American Astronomical Society

Publication Date

July 1, 2011

DOI

10.1088/2041-8205/735/1/l1

ISSN

2041-8205