Title of article
The 2008+ outburst of the Be star 28CMa - a multi-instrument study
Author/Authors
Stan Stefl، نويسنده , , Alex C. Carciofi، نويسنده , , Dietrich Baade، نويسنده , , Thomas Rivinius، نويسنده , , Sebastian Otero، نويسنده , , Jean-Baptiste Le Bouquin، نويسنده , , Juan Fabregat، نويسنده , , Atsuo T. Okazaki، نويسنده , , Fredrik Rantakyr، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2010
Pages
3
From page
430
To page
432
Abstract
Optical and IR spectra, optical to sub-mm photometry, visual imaging polarimetry, and IR high-resolution spectro-interferometry are being used to monitor the new outburst of 28 CMa, which started in 2008 and so far closely resembles previous ones. First modeling based on viscous decretion and focused on constraining the disk viscosity parameter, α, is presented.
Keywords
stars: emission-line , Be , stars: mass loss , stars: circumstellar matter
Journal title
Proceedings of the International Astronomical Union
Serial Year
2010
Journal title
Proceedings of the International Astronomical Union
Record number
667911
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