Publication details
Interactions between supernova ejecta and assymetric circumstellar material
| Authors | |
|---|---|
| Year of publication | 2019 |
| Type | Appeared in Conference without Proceedings |
| MU Faculty or unit | |
| Citation | |
| Description | Progenitors of core-collapse supernovae (SN) may experience enhanced mass loss by stellar winds or outburst episodes shortly before the SN explosion. We study the hydrodynamics of spherical SN explosion into a dense circumstellar medium (CSM) with various non-spherical geometries. We calculate the evolution of thermodynamic quantities in the interaction zone with the ultimate goal of synthesizing supernova light curves and other observables. |