STRUCTURE OF CRAB-NEBULA .2. SPATIAL-DISTRIBUTION OF RELATIVISTIC ELECTRONS

被引：39

作者：

WILSON, AS ^{[1
]}

机构：

[1] MULLARD RADIO ASTRON OBSERV,CAMBRIDGE,ENGLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1972年 / 160卷 / 04期

关键词：

Continuum emission - Crab nebula - Diffusion loss - Energy - Loss model - Relativistic electron;

D O I：

10.1093/mnras/160.4.355

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

A diffusion-loss model is proposed for the Crab Nebula. Relativistic electrons are produced near the centre of the nebula, diffuse outwards and lose energy by synchrotron radiation. Many of the observed features of the continuum emission may be explained in this way. ©Royal Astronomical Society.

引用

页码：355 / 371

页数：17

共 26 条

[1]

ABRAMOWITZ M, 1964, HDB MATHEMATICAL FUN

[2]

BALDWIN JE, 1971, CRAB NEBULA, P22

[3] LUNAR OCCULTATION OF X-RAY EMISSION FROM CRAB NEBULA [J].