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A&A 428, L13-L16 (2004)
DOI: 10.1051/0004-6361:200400095
Letter
First detection of dust clouds around R CrB variable stars
P. de Laverny and D. MékarniaObservatoire de la Côte d'Azur, Dpt Cassiopée, CNRS - UMR 6202, BP 4229, 06304 Nice Cedex 4, France
e-mail: [laverny;mekarnia]@obs-nice.fr
(Received 6 September 2004 / Accepted 23 October 2004 )
Abstract
From VLT/NACO diffraction-limited images of RY Sgr,
we report the first direct detection of heterogeneities
in the circumstellar envelope of a R Coronae Borealis variable star.
Several bright and very large dust clouds are seen in various directions
at several hundred stellar radii from RY Sgr, revealing
high activity for the ejection of stellar material
by R CrB variables.
These observations do support the current
interpretation that optically thick dust clouds are formed
around the surface of this type of variable stars
and, when passing between the star and the observer, produce
the huge and sudden declines characterizing these objects in visible light.
This is the
first direct confirmation of a scenario proposed about 70 years ago.
Key words: stars: AGB and post-AGB -- stars: variables: general -- stars: individual: RY Sgr -- stars: mass-loss -- stars: circumstellar matter -- techniques: high angular resolution
SIMBAD Objects
© ESO 2004
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