Emisión molecular de <SUP>12</SUP>CO en una estrella Be clásica

Las estrellas Be se caracterizan por presentar líneas en emisión de hidrógeno y de metales una vez ionizados, de manera transitoria o permanente. La formación de estas líneas es atribuida a la presencia de una envoltura gaseosa en forma de disco rodeando a la estrella central. A lo largo de la últim...

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Detalles Bibliográficos
Autores principales:	Cochetti, Yanina Roxana, Arias, María Laura, Kraus, M., Cidale, Lydia Sonia, Torres, Andrea Fabiana, Granada, Anahí
Formato:	Articulo
Lenguaje:	Español
Publicado:	2021
Materias:	Ciencias Astronómicas techniques: spectroscopy circumstellar matter stars: emission-line, Be
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/166332
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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