Observations of southern Wolf-Rayet stars - I: The spectroscopic binary HD 90657
The Wolf-Rayet star HD 90657 is found to be a spectroscopic binary with a WN5+O6 spectrum and a period of 6.456 days. Preliminary orbital elements show an elliptic orbit and a mass ratio MWR/Mo∼0.5. Evidence is presented for the Wolf-Rayet atmosphere being accelerated outwards and not being spherica...
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Autor principal: | Niemela, V.S. |
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Formato: | JOUR |
Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_0004640X_v45_n1_p191_Niemela |
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