- 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 usi...
Expand abstract - Publication status:
- Published
- Publisher copy:
- 10.1051/eas/1148096
-
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- Journal:
- CRAL-2010: A UNIVERSE OF DWARF GALAXIES
- Volume:
- 48
- Pages:
- 441-446
- Publication date:
- 2011-01-11
- DOI:
- EISSN:
-
1638-1963
- ISSN:
-
1633-4760
- URN:
-
uuid:8d945ac1-b487-4b2d-99f0-dfcbdf4d9d96
- Source identifiers:
-
205753
- Local pid:
- pubs:205753
- Language:
- English
- Keywords:
- Copyright date:
- 2011
- Notes:
-
Oral Presentation, Proceedings of "A Universe of Dwarf Galaxies"
Conference, Lyon 2010
Journal article
How Does Feedback Affect Milky Way Satellite Formation?
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