DISSIPATION OF MAGNETIC-FIELDS IN VERY DENSE INTERSTELLAR CLOUDS .1. FORMULATION AND CONDITIONS FOR EFFICIENT DISSIPATION

被引:130
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NAKANO, T
UMEBAYASHI, T
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10.1093/mnras/218.4.663
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P1 [天文学];
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0704 ;
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页码:663 / 684
页数:22
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[1]   MAGNETIC STARS [J].
BORRA, EF ;
LANDSTREET, JD ;
MESTEL, L .
ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1982, 20 :191-220
[2]  
Cowling TG., 1957, MAGNETOHYDRODYNAMICS
[4]   On the resistance experienced by spheres in their motion through gases [J].
Epstein, PS .
PHYSICAL REVIEW, 1924, 23 (06) :710-733
[5]  
FIELD GB, 1970, MEM SOC R SCI LIEGE, V59, P29
[6]   THERMAL AND DYNAMICAL EVOLUTION OF GAS CLOUDS OF VARIOUS MASSES [J].
HATTORI, T ;
NAKANO, T ;
HAYASHI, C .
PROGRESS OF THEORETICAL PHYSICS, 1969, 42 (04) :781-&
[7]   STAR FORMATION IN MAGNETIC DUST CLOUDS [J].
MESTEL, L ;
SPITZER, L .
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1956, 116 (05) :503-514
[8]  
Mestel L, 1965, Q J R ASTR SOC, V6, P265
[9]  
NAKANO T, 1985, PUBL ASTRON SOC JPN, V37, P69
[10]  
Nakano T., 1984, Fundamentals of Cosmic Physics, V9, P139