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...

Disgrifiad llawn

Manylion Llyfryddiaeth

Prif Awduron:	Yui Kuboike, Toshiki Sato, Hiromasa Suzuki, Kai Matsunaga, Hiroyuki Uchida, John P. Hughes, Paul P. Plucinsky
Fformat:	Artigo
Iaith:	Inglês
Cyhoeddwyd:	IOP Publishing 2025-01-01
Cyfres:	The Astrophysical Journal
Pynciau:	X-ray astronomy Supernova remnants Massive stars Stellar structures
Mynediad Ar-lein:	https://doi.org/10.3847/1538-4357/ae201e
Tagiau:	Ychwanegu Tag Dim Tagiau, Byddwch y cyntaf i dagio'r cofnod hwn!