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Optical Interferometry of Non-spherical Winds

Published online by Cambridge University Press:  12 April 2016

Farrokh Vakili ,
Denis Mourard ,
Philippe Stee  and
Daniel Bonneau
Farrokh Vakili
Affiliation:
Observatoire de la Côte d’Azur, Presnel-GI2T, F-06460 Caussols, France
Denis Mourard
Affiliation:
Observatoire de la Côte d’Azur, Presnel-GI2T, F-06460 Caussols, France
Philippe Stee
Affiliation:
Observatoire de la Côte d’Azur, Presnel-GI2T, F-06460 Caussols, France
Daniel Bonneau
Affiliation:
Observatoire de la Côte d’Azur, Presnel-GI2T, F-06460 Caussols, France

Abstract

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Optical Long Baseline Interferometry (OLBI) combined with spectral resolution is capable to sounding the stratification of luminous star winds. In this paper we review some few, yet unique results obtained on P Cyg and Be stars from OLBI observations. We also examine the prospects for studying hot stars winds offered by optical synthesis arrays presently under construction.

Type
Section I Observations of Non-spherical Winds
Information
International Astronomical Union Colloquium , Volume 169: Variable and Non-spherical Stellar Winds in Luminous Hot Stars , 1999 , pp. 87 - 94
Copyright
Copyright © Springer-Verlag 1999

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