The Equatorial Expansion of Be stars: A Thin-Line Wind?

Details The Equatorial Expansion of Be stars: A Thin-Line Wind? The Equatorial Expansion of Be stars: A Thin-Line Wind?

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..449d&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 449-450

Astronomy and Astrophysics

Astrophysics

Stars:Be, Circumstellar Matter, Hydrodynamics

Scientific paper

Numerical solutions for the expansion motion equation in the equatiorial
plane of a rotating early type Be star are presented. Decreasing
terminal velocities are obtained as lower values of the radiative
parameterα are used.

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