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Wolf-Rayet Stars with Massive Companions

Published online by Cambridge University Press:  14 August 2015

Philip Massey
Philip Massey*
Affiliation:
Dominion Astrophysical Observatory National Research Council Victoria, B.C., Canada

Extract

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The study of Wolf-Rayet binaries is important for the information we can gleam about the most fundamental property of any star: its mass. In this regard we are very fortunate, since the masses of WR stars can be determined with far greater confidence than can their luminosities, compositions, colors, effective temperatures, etc. By simply measuring the velocities of both components in a WR+0 system, we can find the minimum masses and the mass ratio of the two stars; if we can get some further handle on the orbital inclination, we then know the mass of the WR star directly.

Type
SESSION 4 — OBSERVATIONS OF WOLF-RAYET BINARIES
Information
Symposium - International Astronomical Union , Volume 99: Wolf-Rayet Stars: Observations, Physics, Evolution , 1982 , pp. 251 - 262
Copyright
Copyright © Reidel 1982 

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