Wolf-Rayet stars in the Magellanic clouds. VI: Spectroscopic orbits of WC binaries and implications for W-R evolution
In addition to obtaining spectroscopic orbits for the three largest WC + O binary systems in the LMC, an improved orbit has been determined for the SMC's bright WO + O system. The very short periods noted in two of the LMC binary systems indicate that orbital angular momentum must have been los...
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Veröffentlicht in: | The Astrophysical journal 1990, Vol.348 (1), p.232-241 |
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