Resolving the kinematics of the discs around Galactic B[e] supergiants

B[e] supergiants are luminous evolved massive stars. The mass-loss during this phase creates a complex circumstellar environment with atomic, molecular, and dusty regions usually found in rings or disc-like structures. For a better comprehension of the mechanisms behind the formation of these rings,...

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Detalles Bibliográficos
Autores principales:	Maravelias, G., Kraus, Michael, Cidale, Lydia Sonia, Borges Fernades, M., Arias, María Laura, Curé, Michel, Vasilopoulos, G.
Formato:	Articulo Preprint
Lenguaje:	Inglés
Publicado:	2018
Materias:	Ciencias Astronómicas Stars: circumstellar matter Stars: early-type Stars: massive Stars: supergiants Stars: winds, outflows
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/93487 https://academic.oup.com/mnras/article-abstract/480/1/320/5049025?redirectedFrom=fulltext
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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