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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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| Gepubliceerd in: | Revista Mexicana de Astronomía y Astrofísica |
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| Hoofdauteurs: | , |
| Formaat: | Artigo |
| Taal: | Inglês |
| Gepubliceerd in: |
Universidad Nacional Autónoma de México
2009
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| Onderwerpen: | |
| Online toegang: | https://www.redalyc.org/articulo.oa?id=57112288001 |
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