Modeling of interactions between supernovae ejecta and aspherical circumstellar environments
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DOI: 10.1051/0004-6361/201833429
Abstract: Massive stars are characterized by a significant loss of mass either via spherically symmetric stellar winds or pre-explosion pulses, or by aspherical forms of circumstellar matter (CSM) such as bipolar lobes or outflowing circumstellar equatorial… read more here.
Keywords: interactions supernovae; disk; ejecta aspherical; modeling interactions ... See more keywords