Triggered massive star formation associated with the bubble HII region Sh2-39 (N5)
Aims. We perform a multiwavelength analysis of the bubble Hii region Sh2-39 (N5) and its environs with the aim of studying the physical properties of Galactic IR bubbles and exploring their impact in triggering massive star formation. Methods. To analyze the molecular gas, we used CO(3-2) and HCO&...
Guardado en:
| Autores principales: | Duronea, Nicolás Urbano, Cappa, Cristina Elisabet, Bronfman, L., Borissova, J., Gromadzki, M., Kuhn, M. A. |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2017
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/87432 |
| Aporte de: |
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