Title of article :
Physics and modes of star cluster formation
Author/Authors :
Matthew R. Bate، نويسنده ,
Issue Information :
روزنامه با شماره پیاپی سال 2009
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
Journal title :
Proceedings of the International Astronomical Union
