Services
|
Observing with the VLTI
G. Perrin and F. Malbet (eds)
EAS Publications Series, Vol. 6, 2003
DOI: 10.1051/eas:2003024
The circumstellar disk of the Be star 28 (
) CMa
S. Stefl1, W. Nowotny-Schipper2 and J. Reunanen3
1 Astronomical Institute, Academy of Sciences, Czech Republic;
2 Institut für Astronomie, Universität Wien Austria;
3 Tuorla Observatory, University of Turku;
sstefl@sunstel.asu.cas.cz
nowotny@astro.univie.ac.at
reunanen@astro.utu.fi
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.
© EAS, EDP Sciences 2003
| What is OpenURL? |

Document
BibSonomy
CiteUlike
Connotea
Del.icio.us
Digg
Facebook