Modeling the Structure of Hot Star Disks: a Critical Evaluation of the Viscous Decretion Scenario

UNCG Author/Contributor (non-UNCG co-authors, if there are any, appear on document)
Anatoly S. Miroshnichenko, Professor (Creator)
The University of North Carolina at Greensboro (UNCG )
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Abstract: We present self-consistent solutions for the disk structure of classical Be stars. Our disk model is hydrostatically supported in the vertical direction and the radial structure is governed by viscosity (a-disks). We perform three-dimensional non-LTE Monte Carlo simulations to calculate simultaneously both the equilibrium temperature and Hydrogen level populations and to solve self-consistently for the density structure of the disk. We discuss the general properties of the solution for the disk structure and test our model against observations of d Scorpii. Our results confirm that a viscous decretion disk model is consistent with these observations.

Additional Information

Language: English
Date: 2006
Monte Carlo simulations, hot star, viscous decretion, disk structure

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