ORIGIN OF MAGNETIC-FIELD AND RELATIVISTIC PARTICLES IN CRAB-NEBULA

被引：0

作者：

REES, MF

GUNN, FE

机构：

[1] UNIV SUSSEX,ASTRON CTR,BRIGHTON,ENGLAND

[2] HALE OBSERV,PASADENA,CA

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1974年 / 167卷 / 01期

关键词：

Pulsars - Shellfish - Synchrotron radiation;

D O I：

10.1093/mnras/167.1.1

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

The power from the Crab Pulsar NP 0531 probably emerges partly as 30 Hz waves and partly as a relativistic wind containing a toroidal magnetic field. A shock discontinuity is expected where the pressure of the relativistic outflow balances the pressure within the nebula. This shock would occur at a radius Rs which is about 10 per cent of the total nebular radius Rneb. The relativistic particles and the magnetic flux would accumulate in the region Rs © 1974 Royal Astronomical Society.

引用

页码：1 / 12

页数：12

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