Degeneracies between self-interacting dark matter and supernova feedback as cusp-core transformation mechanisms
Abstract We present a suite of 16 high-resolution hydrodynamic simulations of an isolated dwarf galaxy (gaseous and stellar disk plus a stellar bulge) within an initially cuspy dark matter (DM) halo, including self-interactions between the DM particles (SIDM); as well as stochastic star formation a...
| Main Authors: | , , , , , |
|---|---|
| Format: | Article |
| Language: | English |
| Published: |
Oxford University Press (OUP)
2022
|
| Online Access: | https://hdl.handle.net/1721.1/142385 |