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Title:
Physics and modes of star cluster formation
Authors:
Bate, Matthew R.
Affiliation:
AA(School of Physics, University of Exeter, Stocker Road, Exeter EX4 4QL, UK )
Publication:
Star clusters: basic galactic building blocks throughout time and space, Proceedings of the International Astronomical Union, IAU Symposium, Volume 266, p. 29-34
Publication Date:
01/2010
Origin:
CUP
Keywords:
gravitation, hydrodynamics, MHD, radiative transfer, stellar dynamics, methods: numerical, stars: formation, stars: low-mass, brown dwarfs, stars: luminosity function, mass function
DOI:
10.1017/S1743921309990834
Bibliographic Code:
2010IAUS..266...29B

Abstract

I review the progress made in understanding the physics and modes of star cluster formation through the use of direct self-gravitating hydrodynamical simulations, including those that have recently been performed incorporating radiative transfer and magnetic fields.
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Database: Astronomy
Physics
arXiv e-prints