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...

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Autores principales: Vasquez, Javier, Cappa, Cristina Elisabet, Pineault, Serge, Duronea, Nicolás Urbano
Formato: Articulo
Lenguaje:Inglés
Publicado: 2010
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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
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