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Magnetic fields of massive stars

Published online by Cambridge University Press:  12 July 2011

Swetlana Hubrig ,
Michel Curé ,
Ilya Ilyin  and
Markus Schöller
Swetlana Hubrig
Affiliation:
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, Potsdam, Germany email: [email protected]
Michel Curé
Affiliation:
Departamento de Fisica y Astronomía, Facultad de Ciencias, Universidad de Valparaíso, Chile
Ilya Ilyin
Affiliation:
Astrophysikalisches Institut Potsdam, An der Sternwarte 16, Potsdam, Germany email: [email protected]
Markus Schöller
Affiliation:
European Southern Observatory, Karl-Schwarzschild-Str. 2, 85748 Garching bei München, Germany
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Abstract

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We recently carried out a spectropolarimetric study of a sample of massive O-type stars and pulsating β Cephei stars using the SOFIN echelle spectrograph at the 2.56 m Nordic Optical Telescope and the low-resolution FORS 2 spectrograph at the VLT in spectropolarimetric mode. The sample consists of massive stars already detected as magnetic in the course of our previous low-resolution polarimetric observations with FORS 1 and a few O-type stars with magnetic field detections reported in the literature.

Keywords

stars: magnetic fieldstechniques: polarimetricstars: early-typestars: rotationstars: oscillationsstars: kinematicsstars: individual (HD 108, HD 191612, V1449 Aql, ξ1 CMa)
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. 196 - 197
Copyright
Copyright © International Astronomical Union 2011

References

Belkacem, K., Samadi, R., Goupil, M.-J., Lefèvre, L. et al. 2009, Science 324, 1540CrossRefGoogle Scholar
Donati, J.-F., Howarth, I. D., Bouret, J.-C., Petit, P. et al. 2006, MNRAS 365, L6CrossRefGoogle Scholar
Howarth, I. D., Walborn, N. R., Lennon, D. J., Puls, J. et al. 2007, MNRAS 381, 433CrossRefGoogle Scholar
Hubrig, S., Briquet, M., Schöller, M., De Cat, P. et al. 2006, MNRAS 369, L61CrossRefGoogle Scholar
Hubrig, S., Schöller, M., Schnerr, R. S., González, J. F. et al. 2008, A&A 490, 793Google Scholar
Hubrig, S., Stelzer, B., Schöller, M., Grady, C. et al. 2009a, A&A 502, 283Google Scholar
Hubrig, S., Briquet, M., De Cat, P., Schöller, M. et al. 2009b, AN 330, 317Google Scholar
Martins, F., Donati, J.-F., Marcolino, W. L. F., Bouret, J.-C. et al. 2010, MNRAS 407, 1423CrossRefGoogle Scholar
Nazé, Y., Barbieri, C., Segafredo, A., Rauw, G. et al. 2006, IBVS 5693Google Scholar
Walborn, N. R. 2006, in: The Ultraviolet Universe: Stars from Birth to Death, Proc. IAU Joint Discussion 4, #19, Prague, Czech RepublicGoogle Scholar