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Massive OB stars at varying Z

Published online by Cambridge University Press:  23 January 2015

A. Herrero ,
M. Garcia ,
S. Simón-Díaz ,
I. Camacho ,
C. Sabín-Sanjulián  and
N. Castro
A. Herrero
Affiliation:
Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, E-38200 La Laguna, Spain email: ahd@iac.es Departamento de Astrofísica, Universidad de La Laguna, La Laguna, Spain
M. Garcia
Affiliation:
Centro de Astrobiología, Madrid, CSIC, Spain
S. Simón-Díaz
Affiliation:
Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, E-38200 La Laguna, Spain email: ahd@iac.es Departamento de Astrofísica, Universidad de La Laguna, La Laguna, Spain
I. Camacho
Affiliation:
Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, E-38200 La Laguna, Spain email: ahd@iac.es Departamento de Astrofísica, Universidad de La Laguna, La Laguna, Spain
C. Sabín-Sanjulián
Affiliation:
Departamento de Física, Universidad de La Serena, Chile
N. Castro
Affiliation:
Argelander Institut für Astronomie, Auf dem Hügel 71, 53121 Bonn, Germany
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Abstract

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Massive stars play a key role in environments with very different metallicities. To interpret the role of massive stars in these systems we have to know their properties at different metallicities. The Local Group offers an excellent laboratory to this aim.

Keywords

stars: fundamental parameterssupergiantswindsgalaxies: Local Group
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. 106 - 107
Copyright
Copyright © International Astronomical Union 2015 

References

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