The Future of Theory and Simulation in High-Mass Star Formation

Details The Future of Theory and Simulation in High-Mass Star Formation The Future of Theory and Simulation in High-Mass Star Formation

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aspc..387..306k&link_type=abstract

Massive Star Formation: Observations Confront Theory ASP Conference Series, Vol. 387, proceedings of the conference held 10-14 S

Physics

1

Scientific paper

I discuss the state-of-the-art in modern simulations of high-mass star formation. I elucidate the importance of an accurate formulation of radiation-hydrodynamics and the essential physics required. The discovery of two key mechanisms in fully 3D simulations now points the way to overcome the radiation pressure barrier to high-mass star formation. I outline the future advancements necessary in the theory and simulation of high-mass stars.

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