A Coronagraphic Pilot Study of the Circumstellar Environments around Red Supergiants: CD -31°4916’s Dust Morphology

Many mechanisms have been proposed to contribute to massive-star mass loss, but in general little is known about the physics involved. Studies of circumstellar environments around massive stars might help to determine which mechanisms are the most common. With the recent advent of high-contrast, ext...

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Autores principales:	Jamie R. Lomax, Emily M. Levesque, John P. Wisniewski, John H. Debes
Formato:	Artigo
Lenguaje:	Inglês
Publicado:	IOP Publishing 2025-01-01
Colección:	The Astronomical Journal
Materias:	Stellar mass loss Coronagraphic imaging Circumstellar matter Red supergiant stars
Acceso en línea:	https://doi.org/10.3847/1538-3881/adf83d
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