THE EXPANSION OF A STELLAR WIND BUBBLE WITHIN A NON-SINGULAR, STRATIFIED CORE
We study analytically the expansion of a non-radiative bubble (driven by the wind from a massive star) into an environment with a non-singular, self-gravitating isothermal sphere density stratification. We derive the equation of motion forthe outer radius of the bubble (using the assumptions of th...
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| I publikationen: | Revista Mexicana de Astronomía y Astrofísica |
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| Huvudupphov: | , |
| Materialtyp: | Artigo |
| Språk: | Inglês |
| Utgiven: |
Universidad Nacional Autónoma de México
2012
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| Ämnen: | |
| Länkar: | https://www.redalyc.org/articulo.oa?id=57124423007 |
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