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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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書目詳細資料
發表在:Revista Mexicana de Astronomía y Astrofísica
Principais autores: G. Montes, A. Alberdi, M. A. Pérez-Torres, R. F. González
格式: Artigo
語言:Inglês
出版: Universidad Nacional Autónoma de México 2015
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在線閱讀: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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