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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| Publicat a: | Revista Mexicana de Astronomía y Astrofísica |
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| Autors principals: | , , , |
| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
Universidad Nacional Autónoma de México
2015
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| Matèries: | |
| Accés en línia: | 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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