A magnetohydrodynamical model for the formation of episodic jets

Monthly Notices of the Royal Astronomical Society

Volumn 395, Issue 4, 2009, Pages 2183-2188

  Yuan, Feng ^a   Lin, Jun ^b,c   Wu, Kinwah ^d   Ho, Luis C ^e  

^a INSTITUTE OF GEOLOGY AND GEOPHYSICS   (China)

^b CHINESE ACADEMY OF SCIENCES   (China)

^c HARVARD SMITHSONIAN CENTER FOR ASTROPHYSICS   (United States)

^d UNIVERSITY COLLEGE LONDON   (United Kingdom)

^e CARNEGIE OBSERVATORIES   (United States)

Author keywords

Accretion, accretion discs; Black hole physics; ISM: jets and outflow; MHD

Indexed keywords

BLACK HOLES; GRAVITATION; MAGNETOPLASMA; ROPE; SHEAR FLOW; STARS;

ACCRETION FLOW; ACCRETION: ACCRETION DISKS; BLACK HOLE PHYSICS; BLACK HOLES; CONTINUOUS JETS; FLUX ROPES; HOLE SYSTEMS; ISM JETS AND OUTFLOWS; LARGE-SCALES; MAGNETIC-FIELD;

MAGNETOHYDRODYNAMICS;

EID: 66149175790     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.14673.x     Document Type: Article

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