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- Title
HOW DOES FEEDBACK AFFECT MILKY WAY SATELLITE FORMATION?
- Authors
Geen, S.; Slyz, A.; Devriendt, J.
- Abstract
We use sub-parsec resolution hydrodynamic resimulations of a Milky Way (MW) like galaxy at high redshift to investigate the formation of the MW satellite galaxies. More specifically, we assess the impact of supernova feedback on the dwarf progenitors of these satellite, and the efficiency of a simple instantaneous reionisation scenario in suppressing star formation at the low-mass end of this dwarf distribution. Identifying galaxies in our high redshift simulation and tracking them to z = 0 using a dark matter halo merger tree, we compare our results to present-day observations and determine the epoch at which we deem satellite galaxy formation must be completed. We find that only the low-mass end of the population of luminous subhalos of the Milky-Way like galaxy is not complete before redshift 8.5, and that although supernovae feedback reduces the stellar mass of the low-mass subhalos (M ≤ 109Msun), the number of surviving satellites around the Milky-Way like galaxy at z = 0 is the same in the run with or without supernova feedback. If a luminous halo is able to avoid accretion by the Milky-Way progenitor before redshift 3, then it is likely to survive as a MW satellite to redshift 0.
- Subjects
DIFFUSE ionized gas (Astronomy); GALACTIC coordinates; TIDAL stripping (Astrophysics); DWARF galaxies; STELLAR evolution; ROTATION of galaxies
- Publication
EAS Publications Series, 2011, Vol 48, p441
- ISSN
1633-4760
- Publication type
Article
- DOI
10.1051/eas/1148096