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Inflation of luminous metal-rich WR stars – a clue to mass loss?

Published online by Cambridge University Press:  01 August 2006

Onno R. Pols
Onno R. Pols*
Affiliation:
Sterrenkundig Instituut Utrecht, Postbus 80000, NL-3508TA Utrecht, the Netherlands email: o.r.pols@astro.uu.nl
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Abstract

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We investigate the influence of metallicity and wind mass loss on the radii of luminous Wolf-Rayet stars.

Keywords

stars: mass loss

References

Ishii, M., Ueno, M., & Kato, M. 1999, PASJ, 51, 417CrossRefGoogle Scholar