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Optical Resolution of Be Star Envelopes

Published online by Cambridge University Press:  26 May 2016

F. Vakili ,
D. Mourard  and
P. Stee
F. Vakili
Affiliation:
OCA-Fresnel-GI2T, 06460 Caussols, France
D. Mourard
Affiliation:
OCA-Fresnel-GI2T, 06460 Caussols, France
P. Stee
Affiliation:
OCA-Fresnel-GI2T, 06460 Caussols, France

Abstract

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Probing the atmospheres of Be stars by means of Optical Long Baseline Interferometry (OLBI) is a method still in its infancy. Published observational results in this field can be counted on one hand. In this paper we introduce the principles of OLBI as they apply to observations of Be stars and review results from existing long baseline interferometers. Regular operation of OLBI is most effective when carried out in conjunction with standard techniques such as photometry and spectroscopy. With the next generation of synthetic arrays combining sub-milliarcsecond resolution and a spectral resolution better than 10000, OLBI should be able to address the direct detection of pulsation and magnetic fields.

Type
6. Be Stars: Circumstellar Environment
Information
Symposium - International Astronomical Union , Volume 162: Pulsation, Rotation and Mass Loss in Early-Type Stars , 1994 , pp. 435 - 447
Copyright
Copyright © Kluwer 1994 

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