The 2008+ outburst of the Be star 28 CMa - a multi-instrument study†

Details The 2008+ outburst of the Be star 28 CMa - a multi-instrument study† The 2008+ outburst of the Be star 28 CMa - a multi-instrument study†

Jul 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011iaus..272..430s&link_type=abstract

Active OB stars: structure, evolution, mass loss, and critical limits, Proceedings of the International Astronomical Union, IAU

Astronomy and Astrophysics

Astronomy

1

Stars: Circumstellar Matter, Stars: Emission-Line, Be, Stars: Mass Loss

Scientific paper

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.

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