The fine structures of planetary nebulae

被引：2

作者：

Dyson, JE ^{[1
]}

Hartquist, TW

Redman, MP

Williams, RJR

机构：

[1] Univ Leeds, Dept Phys & Astron, Leeds LS2 9JT, W Yorkshire, England

[2] Univ Manchester, Dept Phys & Astron, Jodrell Bank Observ, Macclesfield SK11 9DL, Cheshire, England

[3] Cardiff Univ, Dept Phys & Astron, Cardiff, S Glam, Wales

来源：

ASTROPHYSICS AND SPACE SCIENCE | 2000年 / 272卷 / 1-3期

关键词：

D O I：

10.1023/A:1002636210925

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Most theoretical studies of the dynamics of planetary nebulae assume that the slow ejecta from the red-giant or asymptotic giant branch phase of evolution of the central star is distributed smoothly. We consider briefly the observational evidence for small scale structure in both neutral and ionised PNe gas, examine some of the ways it can be generated and describe some of the consequences of its presence.

引用

页码：197 / 204

页数：8

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