Instabilities in Hot Star Winds

Details Instabilities in Hot Star Winds Instabilities in Hot Star Winds

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15..228g&link_type=abstract

Winds, Bubbles, and Explosions: a conference to honor John Dyson, Pátzcuaro, Michoacán, México, September 9-13, 2002 (Eds. S. J.

Astronomy and Astrophysics

Astronomy

Radio Continuum: Stars, Stars: Individual (P Cyg, Cyg Ob2 No.12, Wr 147), Stars: Stellar Winds

Scientific paper

We present work investigating the stability of line-driven winds using a
non-Sobolev approach. We find that the dense shell structures that
characterize the growth of radiation-driven instabilities in
one-dimensional simulations break up into numerous bow-shaped clumps in
two dimensions.

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