The Origin of the Mg-rich Supernova Remnant J0550–6823 and the Frequency of Similar Events in the Large Magellanic Cloud

Shell burning and internal mixing in massive stars play an important role in setting the initial conditions for core-collapse supernova explosions. In the late stages of stellar evolution, intense shell burning can cause distinct convective regions to merge, fundamentally restructuring the stellar i...

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Autores principales:	Yui Kuboike, Toshiki Sato, Hiromasa Suzuki, Kai Matsunaga, Hiroyuki Uchida, John P. Hughes, Paul P. Plucinsky
Formato:	Artigo
Lenguaje:	Inglês
Publicado:	IOP Publishing 2025-01-01
Colección:	The Astrophysical Journal
Materias:	X-ray astronomy Supernova remnants Massive stars Stellar structures
Acceso en línea:	https://doi.org/10.3847/1538-4357/ae201e
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