DISKS SURROUNDING MASSIVE STARS: WHEN COMPUTATIONAL MODELS ARE CONFRONTED BY OBSERVATIONS

Many massive stars are embedded within gaseous circumstellar matter; sometimes dust and molecules are also present. Though the disks are sometimes too small to be detected directly, this material can be detected in thespectrum of radiation we observe from the star. Often, the circumstellar material...

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Bibliografische gegevens

Gepubliceerd in:	Revista Mexicana de Astronomía y Astrofísica
Hoofdauteurs:	C. E. Jones, C. Tycner, J. A. Benson, D. J. Hutter, H. R. Schmitt, T. A. A. Sigut, R. T. Zavala
Formaat:	Artigo
Taal:	Inglês
Gepubliceerd in:	Universidad Nacional Autónoma de México 2010
Onderwerpen:	Física, Astronomía y Matemáticas
Online toegang:	https://www.redalyc.org/articulo.oa?id=57115706034
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