The very massive X-ray bright binary system Wack 2134 (= WR 21a)

From the radial velocities of the N IV λ4058 and He II λ4686 emission lines, and the N v λ4604-20 absorption lines, determined in digital spectra, we report the discovery that the X-ray bright emission line star Wack 2134 (= WR 21a) is a spectroscopic binary system with an orbital period of 31.673 ±...

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Detalles Bibliográficos
Autores principales: Niemelä, Virpi Sinikka, Gamen, Roberto, Barbá, Rodolfo Héctor, Fernández Lajús, Eduardo, Benaglia, Paula, Solivella, Gladys Rebeca, Reig, P., Coe, M. J.
Formato: Articulo
Lenguaje:Inglés
Publicado: 2008
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Acceso en línea:http://sedici.unlp.edu.ar/handle/10915/84153
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