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Seven Be stars resolved by optical long-baseline interferometry

Published online by Cambridge University Press:  26 May 2016

A. Quirrenbach
A. Quirrenbach*
Affiliation:
NRL/USNO Optical Interferometer Project and USRA

Extract

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The recent progress in optical interferometry has made the direct study of the circumstellar matter around Be stars possible. The Hα emission region around γ Cas has been resolved with the I2T (Thom et al. 1986), GI2T (Mourard et al. 1989) and MkIII (Quirrenbach et al. 1993) instruments; the results support the basic picture of a rotating disk-shaped envelope (e.g. Poeckert and Marlborough 1978). Nearly spherical geometries can be ruled out. In this paper, first results from MkIII observations of a small sample of Be stars (see Table I) will be presented.

Type
6. Be Stars: Circumstellar Environment
Information
Symposium - International Astronomical Union , Volume 162: Pulsation, Rotation and Mass Loss in Early-Type Stars , 1994 , pp. 450 - 451
Copyright
Copyright © Kluwer 1994 

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