Title of article
Physics and modes of star cluster formation
Author/Authors
Matthew R. Bate، نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2009
Pages
6
From page
29
To page
34
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.
Keywords
mass function , MHD , GRAVITATION , methods: numerical , Stars: luminosity function , stellar dynamics , radiative transfer , stars: formation , stars: low-mass , hydrodynamics , brown dwarfs
Journal title
Proceedings of the International Astronomical Union
Serial Year
2009
Journal title
Proceedings of the International Astronomical Union
Record number
673320
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