Structure and Evolution of Circumstellar Shells Formed by Massive Star Winds

Details Structure and Evolution of Circumstellar Shells Formed by Massive Star Winds Structure and Evolution of Circumstellar Shells Formed by Massive Star Winds

Feb 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995ap%26ss.224..459g&link_type=abstract

Astrophysics and Space Science, Volume 224, Issue 1-2, pp. 459-460

Astronomy and Astrophysics

Astrophysics

Massive Stars, Mass Loss, Lbv-Nebulae, Wr Nebulae

Scientific paper

We follow the interaction of massive stars with their circumstellar gas
over their entire life-times by combining hydrodynamic stellar evolution
calculations for 35 and 60M &sun; stars and one- and
two-dimensional gas dynamical calculations for the circumstellar medium.

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