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Scientist
Wien, Universität, Vienna, Austria
Heidelberg, Universität, Germany
A new numerical model to compute photolysis rates and solar heating with anisotropic scattering in spherical geometry
Protostellar evolution. I - The behaviour of the Eddington factor and the accretion shock
Structure and Stability of Steady Protostellar Accretion Flows - Part Three - Nonlinear Instabilities
Structure and Stability of Steady Protostellar Accretion Flows - Part Two - Linear Stability Analysis
Structure and stability of steady protostellar accretion flows. I.
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