Opacity Problems in Accretion Disks around Young Stellar Objects

Details Opacity Problems in Accretion Disks around Young Stellar Objects Opacity Problems in Accretion Disks around Young Stellar Objects

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992rmxaa..23..235c&link_type=abstract

Revista Mexicana de Astronomia y Astrofisica, 23, 235

Astronomy and Astrophysics

Astronomy

Scientific paper

RESUMEN. Los discos de acrecimiento alrededor de los objetos estelares j6venes son fifos y densos; las fuentes ma's importantes de opacidad provienen del polvo y de las mde'culas. Los calculos de la estructura interna y atmosf6rica y de los espectros sinteticos de' estos discos no han sido satisfactorios hasta ahora debido a la ausencia de datos confiables de opacidad. Se discuten problemas especfficos. ABSTRACT. Accretion disks around young stellar objects are cool and dense; dust and molecules constitute the most important opacity sources. Calculations of internal and atmospheric structure and of synthetic spectra for these disks have been hindered by the lack of appropriate and reliable opacity data. Specific problems are discussed. Key words: ACCRETION - OPACITIES - STARS: PRE-MAIN-SEQUENCE

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