2D calculations of the collapse of magnetized gas cloud

被引:5
作者
Ardeljan, NV
BisnovatyiKogan, GS
Moiseenko, SG
机构
[1] Dept. of Compl. Math. and Cybernet., Moscow State University, Moscow B-234 119899, Vorobjevy gory
关键词
D O I
10.1007/BF00653762
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
2D numerical simulation of the collapse of a rotating magnetized cloud has been done as preliminary investigation of the magnetorotational mechanism of a supernova explosion. Part of the cloud envelope is ejected when magnetic pressure becomes comparable with gas pressure. The mass of the envelope ejected and the energy it carries away are estimated.
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页码:1 / 13
页数:13
相关论文
共 13 条
[1]  
Ardeljan NV, 1996, ASTRON ASTROPHYS SUP, V115, P573
[2]  
ARDELJAN NV, 1987, PROBLEMS CONSTRUCTIO
[3]  
ARDELYAN IV, 1979, ASTRON ZH, V56, P1244
[4]  
Bisnovaty-Kogan G. S., 1970, Astronomicheskii Zhurnal, V47, P813
[5]  
Bisnovatyi-Kogan G. S., 1976, ASTROPHYS SPACE SCI, V41, P321
[6]  
BISNOVATYIKOGAN GS, 1971, SOV ASTRON, V14, P652
[7]  
BISNOVATYIKOGAN GS, 1989, PHYSICAL PROBLEMS TH
[8]  
COURANT R, 1962, METHODS MATH PHYSICS, V2
[9]  
Landau L. D., 1984, ELECTRODYNAMICS CONT
[10]   A NUMERICAL EXAMPLE OF COLLAPSE OF A ROTATING MAGNETIZED STAR [J].
LEBLANC, JM ;
WILSON, JR .
ASTROPHYSICAL JOURNAL, 1970, 161 (02) :541-&