On why discs generate magnetic towers and collimate jets

Monthly Notices of the Royal Astronomical Society

Volumn 341, Issue 4, 2003, Pages 1360-1372

  Lynden Bell, D ^a,b,c,d  

^a CARNEGIE OBSERVATORIES   (United States)

^b UNIVERSITY OF CAMBRIDGE   (United Kingdom)

^c CLARE COLLEGE   (United Kingdom)

^d QUEEN'S UNIVERSITY BELFAST   (United Kingdom)

Author keywords

Accretion, accretion discs; Galaxies: jets; ISM: jets and outflows; MHD; Quasars: general; Stars: formation

Indexed keywords

ASTROPHYSICS;

ACCRETION: ACCRETION DISKS; AMBIENT PRESSURES; ELECTRICAL CONDUCTIVITY; ENERGY THEOREM; GALAXIES JETS; ISM JETS AND OUTFLOWS; MAGNETIC-FIELD; QUASARS:GENERAL; STARS FORMATION;

MAGNETOHYDRODYNAMICS;

EID: 0242330383     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2003.06506.x     Document Type: Article

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