MAGNETOHYDRODYNAMICAL SUPER-NOVA MODEL

被引：0

作者：

MULLER, E ^{[1
]}

HILLEBRANDT, W ^{[1
]}

机构：

[1] MAX PLANCK INST PHYS & ASTROPHYS, FOHRINGER RING 6, D-8000 MUNICH 40, FED REP GER

来源：

ASTRONOMY & ASTROPHYSICS | 1979年 / 80卷 / 02期

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：147 / 154

页数：8

共 15 条

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ARNETT WD, 1978, P SEATTLE C SOURCES

[3]

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[6]

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[7] HERCULES X-1 - 1.24 2ND PULSATION IN HARD X-RAYS [J].

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[8] ARE SUPERNOVA EXPLOSIONS DRIVEN BY MAGNETIC SPRINGS [J].

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NATURE, 1976, 261 (5562) :673-674

[9] A NUMERICAL EXAMPLE OF COLLAPSE OF A ROTATING MAGNETIZED STAR [J].

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[10] MAGNETOHYDRODYNAMIC PHENOMENA IN COLLAPSING STELLAR CORES [J].

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