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Astronomy Colloquium: "Simulating Star Formation in Turbulent Molecular Clouds", Alexei Kritsuk, University of California, San Diego

Event Type
Seminar/Symposium
Sponsor
Astronomy Department
Location
Astronomy 134
Date
Mar 4, 2014   3:45 pm  
Speaker
Alexei Kritsuk, University of California, San Diego
Views
4006
Originating Calendar
Astronomy Colloquium Speaker Calendar

Understanding how molecular clouds form in the interstellar medium and how they evolve to produce dense filaments and cores that eventually give birth to stars is an important unsolved problem in star formation. From a theoretical perspective, star formation is a challenging multi-scale problem that involves

complex nonlinear interactions of gravity, turbulence, magnetic fields, radiation and feedback processes. I shall describe a self-consistent computational framework for modeling molecular cloud formation in the multiphase ISM as a first step to generate realistic initial conditions for star formation. Our approach is based on self-organization in the turbulent ISM and, with only a few control parameters, our numerical experiments successfully reproduce the observed probability distributions of the molecular gas density, thermal pressure, magnetic field strength, as well as the core mass function. I shall briefly discuss the origin of Larson's scaling relations that naturally emerge in the model.

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