X-Ray Emission from interstellar bubbles around Wolf-Rayet stars

Details X-Ray Emission from interstellar bubbles around Wolf-Rayet stars X-Ray Emission from interstellar bubbles around Wolf-Rayet stars

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011rmxac..40..185t&link_type=abstract

XIII Latin American Regional IAU Meeting (Eds. W. J. Henney & S. Torres-Peimbert) Revista Mexicana de Astronomía y Astrofísica (

Astronomy and Astrophysics

Astronomy

Ism: Bubbles, Ism: Kinematics And Dynamics, Stars: Massive, Stars: Mass-Loss

Scientific paper

We study the evolution of the interstellar and circumstellar media around a massive star (M=40~M_&sun;) through radiative-hydrodynamic simulations. The parameters for the stellar wind and ionizing photon rate vary in time depending on the evolutionary phase of the central star. We compare our results with X-ray observations of wind-blown bubbles around Wolf-Rayet stars.

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