THE NATURE OF THE CM-MM EMISSION IN CLOSE WOLF-RAYET BINARIES

The centimeter spectra of Wolf-Rayet (WR) binaries often sh ow a contribu- tion from a wind-wind collision region (WCR) between the sta rs. In short period systems ( ∼ < 1 yr), such a component is expected to be absorbed by the unsho cked winds, losing any effect from its binarity. Recent studies su...

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Veröffentlicht in:	Revista Mexicana de Astronomía y Astrofísica
Hauptverfasser:	G. Montes, A. Alberdi, M. A. Pérez-Torres, R. F. González
Format:	Artigo
Sprache:	Inglês
Veröffentlicht:	Universidad Nacional Autónoma de México 2015
Schlagworte:	Física, Astronomía y Matemáticas
Online-Zugang:	https://www.redalyc.org/articulo.oa?id=57143120007 https://www.redalyc.org/journal/571/57143120007/ https://www.redalyc.org/journal/571/57143120007/html/ https://www.redalyc.org/journal/571/57143120007/57143120007.epub https://www.redalyc.org/journal/571/57143120007/movil
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