X-RAY EMISSION FROM INTERSTELLAR BUBBLES AROUND WOLF-RAYET STARS
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 w...
| Autores: | , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2011 |
| País: | México |
| Institución: | Universidad Nacional Autónoma de México |
| Repositorio: | Redalyc-UNAM |
| OAI Identifier: | oai:redalyc.org:57121297093 |
| Acceso en línea: | https://www.redalyc.org/articulo.oa?id=57121297093 |
| Access Level: | acceso abierto |
| Palabra clave: | Física, Astronomía y Matemáticas ISM mass loss stars bubbles |
| Sumario: | 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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