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...
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| Gepubliceerd in: | Revista Mexicana de Astronomía y Astrofísica |
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| Hoofdauteurs: | , , , , , , , , |
| Formaat: | Artigo |
| Taal: | Inglês |
| Gepubliceerd in: |
Universidad Nacional Autónoma de México
2008
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| Onderwerpen: | |
| Online toegang: | https://www.redalyc.org/articulo.oa?id=57116159031 |
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