High-resolution, near-infrared observations of B[e] supergiants

B[e] supergiants stars are surrounded by disks formed from material released from the central object. To trace the properties of these disks, diverse emission features in the optical and near-infrared can be used. CO band emission is particularly valuable, because it defines the transition region be...

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Detalles Bibliográficos
Autores principales:	Arias, María Laura, Vallverdú, Rodolfo Enrique, Torres, Andrea Fabiana, Kraus, M.
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2021
Materias:	Ciencias Astronómicas stars: early-type circumstellar matter stars: emission-line, Be
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/167789
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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