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

Toalá J. A.; Arthur S. J.

Vol. 40 No. 1 (2011), Contributions

Vol. 40 No. 1 (2011)

Contributions

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

Toalá J. A.⁺⁻
Arthur S. J.⁺⁻

Toalá J. A.

Centro de Radioastronomía y Astrofísica, Universidad Nacional Autónoma de México, Apdo. Postal 3-72, 58090, Morelia, Michoacán, Mexico

Arthur S. J.

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0000-0002-5456-4472

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Keywords

ISM: bubbles
ISM: kinematics and dynamics
stars: massive
stars: mass-loss

How to Cite

X-Ray Emission from interstellar bubbles around Wolf-Rayet stars. (2011). Revista Mexicana De Astrofísica Y Astronomía Serie De Conferencias, 40(1), 185-186. https://astronomia.unam.mx/journals/rmxac/article/view/2011rmxac..40..185t

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Abstract

We study the evolution of the interstellar and circumstellar media around a massive star (M=40~M_⊙) 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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X-Ray Emission from interstellar bubbles around Wolf-Rayet stars

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