Progenitor Constraint-incorporating Shell Merger: The Case of Supernova Remnant G359.0–0.9

It is generally hard to put robust constraints on progenitor masses of supernovae and supernova remnants (SNRs) observationally, while they offer tantalizing clues to understanding explosion mechanisms and mass distribution. Our recent study suggests that “shell merger,” which is theoretically expec...

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Hlavní autoři:	Kai Matsunaga, Hiroyuki Uchida, Rei Enokiya, Toshiki Sato, Ryo Sawada, Hideyuki Umeda, Takuto Narita, Takeshi Go Tsuru
Médium:	Artigo
Jazyk:	Inglês
Vydáno:	IOP Publishing 2024-01-01
Edice:	The Astrophysical Journal
Témata:	Supernova remnants Molecular clouds Core-collapse supernovae Stellar structures Supernovae Ejecta
On-line přístup:	https://doi.org/10.3847/1538-4357/ad5284
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