Dwarf galaxy formation with and without dark matter-baryon streaming velocities
Anna T. P. Schauer, Michael Boylan-Kolchin, Katelyn Colston, Omid, Sameie, Volker Bromm, James S. Bullock, and Andrew Wetzel

TL;DR
This study investigates how baryon-dark matter streaming velocities influence early dwarf galaxy formation using cosmological hydrodynamic simulations, finding initial delays and suppression effects that diminish by redshift 5.
Contribution
It is the first detailed simulation-based analysis of the impact of baryon-dark matter streaming velocities on dwarf galaxy formation at high redshift.
Findings
Star formation delayed by ~50 Myr in streaming simulations
Number of luminous galaxies suppressed at high redshift in streaming runs
Effects of streaming velocities diminish by redshift 5, with galaxies showing similar properties at z=0
Abstract
We study how supersonic streaming velocities of baryons relative to dark matter -- a large-scale effect imprinted at recombination and coherent over Mpc scales -- affects the formation of dwarf galaxies at . We perform cosmological hydrodynamic simulations, including and excluding streaming velocities, in regions centered on halos with M; the simulations are part of the Feedback In Realistic Environments (FIRE) project and run with FIRE-3 physics. Our simulations comprise many thousands of systems with halo masses between M and M in the redshift range . A few hundred of these galaxies form stars and have stellar masses ranging from 100 to M. While star formation is globally delayed by approximately 50 Myr in the streaming relative to…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Dark Matter and Cosmic Phenomena · Cosmology and Gravitation Theories
