THE FIRST ORBITAL SOLUTION FOR THE MASSIVE COLLIDING-WIND BINARY HD 93162 (-WR 25)
Since the discovery, with EINSTEIN, of strong X-ray emission associated with HD 93162, this object was recurrently predicted by some authors to be a colliding-wind binary system. However, radial velocity variations that would prove the suspected binary nature have never been found so far. We spectro...
Guardado en:
| Publicado en: | Revista Mexicana de Astronomía y Astrofísica |
|---|---|
| Autores principales: | , , , , , , , , |
| Formato: | Artigo |
| Lenguaje: | Inglês |
| Publicado: |
Universidad Nacional Autónoma de México
2008
|
| Materias: | |
| Acceso en línea: | https://www.redalyc.org/articulo.oa?id=57116159031 |
| Etiquetas: |
Sin Etiquetas, Sea el primero en etiquetar este registro!
|