3D Gray Radiative Properties of Accretion Shocks in Young Stellar Objects

3D Gray Radiative Properties of Accretion Shocks in Young Stellar Objects

We address the problem of the contribution of radiation to the structure and dynamics of accretion shocks on Young Stellar Objects. Solving the 3D RTE (radiative transfer equation) under our “gray LTE approach”, i.e., using appropriate mean opacities computed in local thermodynamic equilibrium, we p...

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Bibliographic Details
Main Authors:	Ibgui L., Orlando S., Stehlé C., Chièze J.-P., Hubeny I., Lanz T., de Sá L., Matsakos T., González M., Bonito R.
Format:	Article
Language:	English
Published:	EDP Sciences 2014-01-01
Series:	EPJ Web of Conferences
Online Access:	http://dx.doi.org/10.1051/epjconf/20136404005

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