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RADIO PROPER MOTIONS OF WOLF-RAYET STARS

We present the analysis of observations taken from the Very Large Array archive of sixWolf-Rayet stars with radio emission, with the purpose of determining their proper motions. Typically, these observations cover periods of 10 to 20 years. To verify the method, we included WR 140 in the sample, and...

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Detalles Bibliográficos
Publicado en:Revista Mexicana de Astronomía y Astrofísica
Principais autores: S. Dzib, L. F. Rodríguez
Formato: Artigo
Idioma:Inglês
Publicado: Universidad Nacional Autónoma de México 2009
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Acceso en liña:https://www.redalyc.org/articulo.oa?id=57112288001
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