Evidence for Type Ib/c Origin of the Supernova Remnant G292.0+1.8

Evidence for Type Ib/c Origin of the Supernova Remnant G292.0+1.8

Circumstellar material (CSM) produced by mass loss from massive stars (≳10 M _⊙ ) through strong stellar winds or binary stripping provides rich information for understanding progenitors of core-collapse supernova remnants. In this paper we present a grating spectroscopy of a Galactic SNR G292.0+1.8...

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Bibliographic Details
Main Authors: Takuto Narita, Hiroyuki Uchida, Jacco Vink, Satoru Katsuda, Hideyuki Umeda, Takashi Yoshida, Toshiki Sato, Kai Matsunaga, Takeshi Go Tsuru
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Supernova remnants
Stellar evolution
Circumstellar matter
High energy astrophysics
X-ray sources
Online Access:https://doi.org/10.3847/1538-4357/ad7e17
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https://doi.org/10.3847/1538-4357/ad7e17

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