Observations and Analysis of Be Star Circumstellar Environments with the Long Baseline CHARA Array Interferometer

Details Observations and Analysis of Be Star Circumstellar Environments with the Long Baseline CHARA Array Interferometer Observations and Analysis of Be Star Circumstellar Environments with the Long Baseline CHARA Array Interferometer

Feb 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010rmxac..38..106t&link_type=abstract

The Interferometric View on Hot Stars (Eds. Th. Rivinius & M. Curé) Revista Mexicana de Astronomía y Astrofísica (Serie de Confe

Astronomy and Astrophysics

Astronomy

Cepheids, Stars: Circumstellar Matter, Stars: Mass Oss

Scientific paper

We present our approach in studying and determining the physical and geometrical properties of the circumstellar disks around Be stars. We use observational results on several Be stars obtained with the long baseline CHARA Array interferometer in the K-band. We were able to define for each case the envelope characteristics (projected shape and orientation) and to constrain the gas density and temperature profile interferometrically.

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