FORMATION OF FILAMENTS IN THE CRAB-NEBULA BY A THERMAL SYNCHROTRON INSTABILITY

被引：14

作者：

DALPINO, EMD

OPHER, R

机构：

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1989年 / 240卷 / 03期

关键词：

D O I：

10.1093/mnras/240.3.573

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：573 / 590

页数：18

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[5]

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[8] SPONTANEOUS FORMATION OF KNOTS IN RELATIVISTIC FLOWS - A MODEL FOR VARIABILITY IN COMPACT SYNCHROTRON SOURCES [J].

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ASTROPHYSICAL JOURNAL, 1980, 239 (01) :296-304

[9] SPECTROPHOTOMETRY OF FILAMENTS IN CRAB-NEBULA [J].

MILLER, JS .

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[10]

PIDDINGTON JH, 1957, AUSTR J PHYS, V10, P530

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