Satellite survival in highly resolved Milky Way class haloes
Surprisingly little is known about the origin and evolution of the Milky Way's satellite galaxy companions. UV photoionisation, supernova feedback and interactions with the larger host halo are all thought to play a role in shaping the population of satellites that we observe today, but there...
Autori principali: | Geen, S, Slyz, A, Devriendt, J |
---|---|
Natura: | Journal article |
Pubblicazione: |
Oxford University Press
2012
|
Documenti analoghi
-
How Does Feedback Affect Milky Way Satellite Formation?
di: Geen, S, et al.
Pubblicazione: (2011) -
Modelling the Milky Way stellar halo
di: Fermani, F
Pubblicazione: (2013) -
The Huge Magnetic Toroids in the Milky Way Halo
di: J. Xu, et al.
Pubblicazione: (2024-01-01) -
Angular momentum transfer to a Milky Way disk at high redshift
di: Tillson, H, et al.
Pubblicazione: (2015) -
ELVES. IV. The Satellite Stellar-to-halo Mass Relation Beyond the Milky Way
di: Shany Danieli, et al.
Pubblicazione: (2023-01-01)