Protostars and Planets VI, Heidelberg, July 15-20, 2013
Simulating Shock Triggered Star Formation with AstroBEAR2.0
Li, Shule (Department of Physics and Astronomy, University of Rochester)
Frank, Adam (Department of Physics and Astronomy, University of Rochester)
Blackman, Eric (Department of Physics and Astronomy, University of Rochester)
Star formation can be triggered by the compression from shocks running over stable clouds. Triggered star formation is a favored explanation for the traces of SLRI\'s in our solar system. Previous research has shown that when parameters such as shock speed are within a certain range, the gravitational collapse of otherwise stable, dense cloud cores is possible. However, these studies usually focus on the precursors of star formation, and the conditions for the triggering. We use AstroBEAR2.0 code to simulate the collapse and subsequent evolution of a stable Bonnor-Ebert cloud by an incoming shock. Through our simulations, we show that interesting physics happens when the newly formed star interacts with the cloud residue and the post-shock flow. We identify these interactions as controlled by the initial conditions of the triggering and study the flow pattern as well as the evolution of important physics quantities such as accretion rate and angular momentum.
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