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Asteroseismology of OB stars with hundreds of single snapshot spectra (and a few time-series of selected targets)

Published online by Cambridge University Press:  23 January 2015

S. Simón-Díaz
S. Simón-Díaz*
Affiliation:
Instituto de Astrofísica de Canarias, 38200 La Laguna, Tenerife, Spain email: [email protected] Departamento de Astrofísica, Universidad de La Laguna, 38205 La Laguna, Tenerife, Spain
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Abstract

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Imagine we could do asteroseismology of large samples of OB-type stars by using just one spectrum per target. That would be great! But this is probably a crazy and stupid idea. Or maybe not. Maybe we have the possibility to open a new window to investigate stellar oscillations in massive stars that has been in front of us for many years, but has not attracted very much our attention: the characterization and understanding of the so-called macroturbulent broadening in OB-type stars.

Keywords

stars: early-typestars: oscillations (including pulsations)line: profilestechniques: spectroscopic
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Issue S307: New windows on massive stars: asteroseismology, interferometry, and spectropolarimetry , June 2014 , pp. 194 - 199
Copyright
Copyright © International Astronomical Union 2015 

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