Numerical Simulations of the Interaction of Colliding Stellar Winds with the ISM

Details Numerical Simulations of the Interaction of Colliding Stellar Winds with the ISM Numerical Simulations of the Interaction of Colliding Stellar Winds with the ISM

Jan 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003rmxac..15...83s&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

1

Planetary Nebula, Ism: Jets And Outflows

Scientific paper

We investigate the effects of colliding winds on interstellar bubbles. We present the results of numerical simulations of a bubble that is formed by two close (not binary) stars with strong winds. The two winds will collide and form a thick shocked layer with hot, dense material. The edge of the bubble will be shaped by the undisturbed winds and the impact of the wind-wind shock layer on the interstellar medium (ISM).

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