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Pulsations in massive stars: effect of the atmosphere on the strange mode pulsations

Published online by Cambridge University Press:  12 July 2011

Mélanie Godart ,
Marc-Antoine Dupret ,
Arlette Noels ,
Conny Aerts ,
Sergio Simón-Díaz ,
Karolien Lefever ,
Joachim Puls ,
Josefina Montalban  and
Paolo Ventura
Mélanie Godart
Affiliation:
Astrophysics, Geophysics, and Oceanography Department, University of Liége, Belgium email: godart@astro.ulg.ac.be
Marc-Antoine Dupret
Affiliation:
Astrophysics, Geophysics, and Oceanography Department, University of Liége, Belgium email: godart@astro.ulg.ac.be
Arlette Noels
Affiliation:
Astrophysics, Geophysics, and Oceanography Department, University of Liége, Belgium email: godart@astro.ulg.ac.be
Conny Aerts
Affiliation:
Instituut voor Sterrenkunde, KULeuven, Belgium
Sergio Simón-Díaz
Affiliation:
Instituto de Astrofísica de Canarias, E-38200, La Laguna, Tenerife, Spain Departamento de Astrofísica, Universidad de La Laguna, E-38205 La Laguna, Tenerife, Spain
Karolien Lefever
Affiliation:
Belgisch Instituut voor Ruimte Aeronomie (BIRA), Brussels, Belgium
Joachim Puls
Affiliation:
Universitäts-Sternwarte, Scheinerstrasse 1, 81679 München, Germany
Josefina Montalban
Affiliation:
Astrophysics, Geophysics, and Oceanography Department, University of Liége, Belgium email: godart@astro.ulg.ac.be
Paolo Ventura
Affiliation:
INAF Osservatorio Astronomico di Roma, Monteporzio, Italy
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Abstract

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Recent space observations with CoRoT and ground-based spectroscopy have shown the presence of different types of pulsations in OB stars. These oscillations could be due to acoustic and gravity modes, solar-like oscillations or even other pulsations of large growth rates. We present a first attempt at interpreting the latter as strange modes.

Keywords

stars: atmospheresstars: mass lossstars: oscillations (including pulsations)
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 6 , Symposium S272: Active OB stars: structure, evolution, mass loss, and critical limits , July 2010 , pp. 503 - 504
Copyright
Copyright © International Astronomical Union 2011

References

Aerts, C., Lefever, K., Baglin, A., & Degroote, P. et al. 2010, A&A, 513, L11Google Scholar
Dupret, M.-A., De Ridder, J., Neuforge, C., & Aerts, C. et al. 2002, A&A, 385, 563Google Scholar
Godart, M., Dupret, M.-A., & Noels, A., et al. 2010, AN, in pressGoogle Scholar
Puls, J., Urbaneja, M. A., Venero, R., Repolust, T. et al. 2005, A&A, 435, 669Google Scholar
Ventura, P., D'Antona, F., & Mazzitelli, I. 2008, Ap&SS, 316, 93Google Scholar
Saio, H., Baker, N. H., & Gautschy, A. 1998, MNRAS, 294, 622CrossRefGoogle Scholar