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 ±...
Guardado en:
| 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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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/84153 |
| Aporte de: |
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