The HII Regions and Bow Shocks Around Runaway o Stars
We present a model for the HII region and stellar wind bow shock formed by runaway O stars passing through the Galactic disk. We develop a quasi-analytic approach in which the absorption of stellar ionizing photons by the bow shock is considered. With these models we study the transition between a d...
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| Pubblicato in: | Revista Mexicana de Astronomía y Astrofísica |
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| Autori principali: | , , |
| Natura: | Artigo |
| Lingua: | Inglês |
| Pubblicazione: |
Universidad Nacional Autónoma de México
2022
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| Soggetti: | |
| Accesso online: | https://www.redalyc.org/articulo.oa?id=57175502018 https://www.redalyc.org/journal/571/57175502018/ https://www.redalyc.org/journal/571/57175502018/html/ https://www.redalyc.org/journal/571/57175502018/57175502018.epub https://www.redalyc.org/journal/571/57175502018/movil |
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