Stellar formation in HI interstellar bubbles around massive stars
Stellar winds from O and WR stars transfer large amounts of mechanical energy and momentum into the interstellar medium. They sweep up and compress the interstellar material, creating interstellar bubbles. These structures are detected as optical ring nebulae, as thermal radio continuum sources, as...
| Autores principales: | Martín, María Cristina, Romero, Gisela Andrea, Cappa, Cristina Elisabet |
|---|---|
| Formato: | Articulo Comunicacion |
| Lenguaje: | Inglés |
| Publicado: |
2006
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/83089 |
| Aporte de: |
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