机构:
Univ Calif San Diego, La Jolla, CA 92093 USAUniv Calif San Diego, La Jolla, CA 92093 USA
Kritsuk, Alexei G.
[1
]
Ustyugov, Sergey D.
论文数: 0引用数: 0
h-index: 0
机构:Univ Calif San Diego, La Jolla, CA 92093 USA
Ustyugov, Sergey D.
Norman, Michael L.
论文数: 0引用数: 0
h-index: 0
机构:
Univ Calif San Diego, La Jolla, CA 92093 USAUniv Calif San Diego, La Jolla, CA 92093 USA
Norman, Michael L.
[1
]
机构:
[1] Univ Calif San Diego, La Jolla, CA 92093 USA
来源:
COMPUTATIONAL STAR FORMATION
|
2011年
/
270期
关键词:
ISM: structure;
ISM: clouds;
ISM: magnetic fields;
turbulence;
methods: numerical;
HIGH-RESOLUTION SIMULATIONS;
GALACTIC MOLECULAR CLOUDS;
WARM NEUTRAL MEDIUM;
H I FLOWS;
SUPERSONIC TURBULENCE;
ISOTHERMAL TURBULENCE;
SELF-ORGANIZATION;
MAGNETIC-FIELD;
POWER SPECTRUM;
MHD TURBULENCE;
D O I:
10.1017/S1743921311000342
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
We provide a brief overview of recent advances and outstanding issues in simulations of interstellar turbulence, including isothermal models for interior structure of molecular clouds and larger-scale multiphase models designed to simulate the formation of molecular clouds. We show how self-organization in highly compressible magnetized turbulence in the multiphase ISM can be exploited in simple numerical models to generate realistic initial conditions for star formation.