Ionized gas, molecules and dust in Sh2-132
We analyse the various interstellar components of the H II region Sh2-132. The main stellar source is the double binary system that includes the Wolf–Rayet star WR 153ab. We use radio continuum images at 408 and 1420 MHz, and H I 21-cm line data taken from the Canadian Galactic Plane Survey, molecul...
Guardado en:
| Autores principales: | Vasquez, Javier, Cappa, Cristina Elisabet, Pineault, Serge, Duronea, Nicolás Urbano |
|---|---|
| Formato: | Articulo |
| Lenguaje: | Inglés |
| Publicado: |
2010
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| Materias: | |
| Acceso en línea: | http://sedici.unlp.edu.ar/handle/10915/99133 https://ri.conicet.gov.ar/11336/6315 http://mnras.oxfordjournals.org/content/405/3/1976 |
| Aporte de: |
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