Institute for Astrophysics, University Vienna

After completing my Phd at the Sterrenkundig Instituut Utrecht on "Modeling Populations of Rotationally Mixed Massive Stars" in Feb. 2011, I started a Postdoc at the University of Vienna in Jan. 2011.
Here I will concentrate on simulations of stellar discs (in particular t-tauri discs) with the 3D-radiative transfer code PHOENIX.

Downloads Evolutionary models and Isochrones of rotating massive stars, published in Brott et. al 2011a can be downloaded here

Press Releases

• Snelle rotatie nie alleen bepalend voor mengprocess in zware sterren
• VLT Finds Fastest Rotating Star

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