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Polarimetric Evidence of Non-Spherical Winds

Antonio Mario Magalhaes·Claudia V. Rodrigues
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Abstract

Polarization observations yield otherwise unobtainable information about the geometrical structure of unresolved objects. In this talk we review the evidences for non-spherically symmetric structures around Luminous Hot Stars from polarimetry and what we can learn with this technique. Polarimetry has added a new dimension to the study of the envelopes of Luminous Blue Variables, Wolf-Rayet stars and B[e] stars, all of which are discussed in some detail.

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BibTeXRIS

Antonio Mario Magalhaes, Claudia V. Rodrigues. 1999-02-04. Polarimetric Evidence of Non-Spherical Winds. https://doi.org/10.1007/bfb0106354

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