Massive Star Formation Near the Supernova Remnant W30
We present arcsecond-resolution 6 cm continuum observations of potentialmassive-star formation sites in the vicinity of the W30 supernova remnant. Ninesources are detected, several of which could be ultracompact H II regions. Oneof these, G8.139-0:026 has a cometary morphology. Of the eight IRAS sou...
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| Publié dans: | Revista Mexicana de Astronomía y Astrofísica |
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| Auteurs principaux: | , , , , |
| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
Universidad Nacional Autónoma de México
2002
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| Sujets: | |
| Accès en ligne: | https://www.redalyc.org/articulo.oa?id=57138111 |
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