The Stellar Wind from MWC349A

Details The Stellar Wind from MWC349A The Stellar Wind from MWC349A

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002aas...20114404g&link_type=abstract

American Astronomical Society Meeting 201, #144.04; Bulletin of the American Astronomical Society, Vol. 35, p.570

Astronomy and Astrophysics

Astronomy

Scientific paper

Radio recombination lines determine the radial gas flow from the star MWC349A. The flow is described by a beta law with β =5, a terminal velocity of 34 km/s, and a mass loss of approximately 10-6 solar masses per year. Such a flow could also be the result of evaporation from the circumstellar disk surrounding the star. The implied recession velocity of MWC349A is approximately 12 km/s.

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