Molecular environment of the yellow hypergiant star HD 269953

Las hipergigantes amarillas son estrellas masivas, probablemente en una etapa evolutiva posterior a la de supergigante roja. En esta fase, se suelen dar eventos de pérdida de masa, en los cuales el material eyectado forma envolturas de gas y polvo alrededor de la estrella. HD 269953 fue sugerida com...

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Detalles Bibliográficos
Autores principales:	Kraus, M., Arias, María Laura, Cidale, Lydia Sonia, Torres, Andrea Fabiana, Kourniotis, M.
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2022
Materias:	Ciencias Astronómicas stars: massive supergiants circumstellar matter
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/168215
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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