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Spectroscopic versus evolutionary masses

Published online by Cambridge University Press:  01 August 2006

Artemio Herrero
Artemio Herrero*
Affiliation:
Instituto de Astrofisica de Canarias, C/ Via Lactea s/n, E-38200, La Laguna, Tenerife, Spain email: [email protected]
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Abstract

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We describe the present status of the mass discrepancy in the Upper HR Diagram.

Keywords

stars: fundamental parameters (masses)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 201
Copyright
Copyright © International Astronomical Union 2007

References

Herrero, A., Kudritzki, R.-P., Vilchez, J. M., et al. 1992, A&A, 261, 209Google Scholar
Herrero, A., & Lennon, D. J. 2004, in: Maeder, A. & Eenens, P. (eds.), Steller Rotation, Proc. IAU Symp. No. 215 (San Francisco: ASP), p. 209Google Scholar
Mokiem, R. M. 2006, PhD thesis, University of AmsterdamGoogle Scholar
Repolust, T., Puls, J., & Herrero, A. 2004, A&A, 415, 349Google Scholar