Physics
Scientific paper
Apr 2000
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aps..aprh14003o&link_type=abstract
American Physical Society, April Meeting, April 29-May 2, 2000 Long Beach, CA, abstract #H14.003
Physics
Scientific paper
Hot, massive, luminous have very strong stellar winds, with flow speeds
of order 1% the speed of light and mass loss rates sometimes a billion
times that of the solar wind. In this talk, I will review the physics of
how these winds are driven by line-scattering of the star's light, and
contrast this to the gas-pressure driving of the solar wind.
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