The first orbital solution for the massive colliding-wind binary HD 93162 (≡WR 25)

Context. Since the discovery, with the EINSTEIN satellite, of strong X-ray emission associated with HD 93162 (≡WR 25), this object has been predicted to be a colliding-wind binary system. However, radial-velocity variations that would prove the suspected binary nature have yet to be found. Aims. We...

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Autores principales: Gamen, Roberto Claudio, Gosset, E., Morrell, Nidia Irene, Niemelä, Virpi Sinikka, Sana, H., Nazé, Y., Rauw, G., Barbá, Rodolfo Héctor, Solivella, Gladys Rebeca
Formato: Articulo
Lenguaje:Inglés
Publicado: 2006
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/83059
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