MAGNETOHYDRODYNAMIC STABILITY OF WHITE-DWARFS AND NEUTRON STARS

被引:21
作者
TAYLER, RJ [1 ]
机构
[1] UNIV SUSSEX,ASTRON CTR,BRIGHTON BN1 9QH,SUSSEX,ENGLAND
关键词
D O I
10.1093/mnras/162.1.17
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
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页码:17 / 23
页数:7
相关论文
共 11 条
[1]   MONTE CARLO STUDY OF A 1-COMPONENT PLASMA .I. [J].
BRUSH, SG ;
SAHLIN, HL ;
TELLER, E .
JOURNAL OF CHEMICAL PHYSICS, 1966, 45 (06) :2102-+
[3]  
HUBBARD WB, 1968, LOW LUMINOSITY STARS
[4]  
MARKEY PM, IN PRESS
[5]  
MESTEL L, 1971, Q J ROY ASTRON SOC, V12, P402
[6]   ENERGY CONTENT OF A WHITE DWARF AND ITS RATE OF COOLING [J].
MESTEL, L ;
RUDERMAN, MA .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1967, 136 (01) :27-&
[7]   PULSARS - STRUCTURE AND DYNAMICS [J].
RUDERMAN, M .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1972, 10 :427-&
[8]   ADIABATIC STABILITY OF STARS CONTAINING MAGNETIC-FIELDS .1. TOROIDAL FIELDS [J].
TAYLER, RJ .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1973, 161 (04) :365-380
[9]  
Vandakurov Yu. V., 1972, SOV ASTRON, V16, P265
[10]  
WRIGHT GA, IN PRESS