Abstract
We have constructed a versatile new simulation system for studying the small-scale physics of star formation (SF) and feedback within single and interacting galaxies, with an emphasis upon attempting to model the molecular clouds and their interaction with the ISM in a realistic fashion. Our model is fully self-gravitating with optional SPH. In order to attempt to ascertain the primary method of star formation within a galaxy, we have implemented models based upon:
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References
Baxter, Keith, Alexander, Paul, in preparation.
Kwan, J., Valdes, F. 1986, ApJ. 315, 92
Sleath, J., Alexander, P. 1995 MNRAS, 275, 507
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© 1999 Springer Science+Business Media Dordrecht
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Baxter, K., Alexander, P. (1999). Studying the Physics of Star Formation in Single and Interacting Galaxies. In: Miyama, S.M., Tomisaka, K., Hanawa, T. (eds) Numerical Astrophysics. Astrophysics and Space Science Library, vol 240. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-4780-4_33
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DOI: https://doi.org/10.1007/978-94-011-4780-4_33
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