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On the Chemical Abundances, Evolutionary Stage and Bolometric Magnitude of WR Stars
Published online by Cambridge University Press: 14 August 2015
Extract
I will comment on 3 problems concerning WR stars:
a. are WR stars core hydrogen/core helium burning?
b. are WR stars H-poor or do they have normal abundances?
c. can we use B.C. for WR stars which are similar as for 0 stars?
- Type
- SESSION 2 — THE CHEMISTRY OF THE WOLF-RAYET STARS
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- Copyright
- Copyright © Reidel 1982