The kinematic signature of a binary central star in the collimated ejections of planetary nebulae
Binary stars are believed to be involved in some way in the formation of many collimated outows observedin planetary nebulae. The direct detection of binary central stars is observationally dicult, so that indirectmethods o er an interesting alternative for inferring the presence of a binary. It has...
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| Publicado no: | Revista Mexicana de Astronomía y Astrofísica |
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| Autor principal: | |
| Formato: | Artigo |
| Idioma: | Inglês |
| Publicado em: |
Universidad Nacional Autónoma de México
2002
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| Acesso em linha: | https://www.redalyc.org/articulo.oa?id=57101328 |
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