THE WINDS OF THE MOST MASSIVE STARS AS VIEWED FROM LONG-BASELINE INTERFEROMETRY: MODEL PREDICTIONS
Long-baseline interferometry is one of the only techniques capable of providing milli-arcsecond spatial resolution observations which are needed to resolve the winds of massive stars. We present predictions of the interferometric observables of massive stars based on the non-LTE radiative transfer c...
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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
2010
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| Assuntos: | |
| Acesso em linha: | https://www.redalyc.org/articulo.oa?id=57115706017 |
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