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The circumstellar disk of the Be star 28 (ω) CMa

Published online by Cambridge University Press:  31 January 2003

G. Perrin ,
F. Malbet ,
S. Štefl ,
W. Nowotny-Schipper  and
J. Reunanen
S. Štefl*
Affiliation:
Astronomical Institute, Academy of Sciences, Czech Republic;
W. Nowotny-Schipper
Affiliation:
Institut für Astronomie, Universität Wien Austria;
J. Reunanen
Affiliation:
Tuorla Observatory, University of Turku;
*
sstefl@sunstel.asu.cas.cznowotny@astro.univie.ac.atreunanen@astro.utu.fi
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Abstract

We propose interferometric observations of the Be star 28 CMa. Constraints on the geometrical and physical parameters of the disk could be obtained by combining three VLTI auxiliary telescopes.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 6: Observing with the VLTI , 2003 , pp. 257
Copyright
© EAS, EDP Sciences, 2003

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