Non-synchronous rotations in massive binary systems: HD 93343 revisited

<i>Context</i>. Most massive stars are in binary or multiple systems. Several massive stars have been detected as double-lined spectroscopic binaries and among these, the OWN Survey has detected a non-negligible number whose components show very different spectral line broadening (i.e.,...

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Detalles Bibliográficos
Autores principales:	Putkuri, Cristina Ester, Gamen, Roberto Claudio, Morrell, Nidia Irene, Simón Díaz, S., Barbá, Rodolfo Héctor, Ferrero Sosa, Gabriel Antonio, Arias, Julia Inés, Solivella, Gladys Rebeca
Formato:	Articulo Preprint
Lenguaje:	Inglés
Publicado:	2018
Materias:	Astronomía Física Ciencias Naturales Ciencias Exactas Binaries: spectroscopic Stars: early-type Stars: rotation Stars: individual: HD 93343
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/93844 https://www.aanda.org/10.1051/0004-6361/201833574 https://arxiv.org/abs/1810.02154v1
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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