Global non-axisymmetric perturbation configurations in a composite disc system with an isopedic magnetic field: Relation between dark matter halo and magnetic field

Monthly Notices of the Royal Astronomical Society

Volumn 397, Issue 2, 2009, Pages 815-836

  Xiang Gruess, Meng ^a   Lou, Yu Qing ^b,c   Duschl, Wolfgang J ^a,d  

^a UNIVERSITY OF KIEL   (Germany)

^b TSINGHUA UNIVERSITY   (China)

^c CHINESE ACADEMY OF SCIENCES   (China)

^d UNIVERSITY OF ARIZONA   (United States)

Author keywords

Galaxies: haloes; Galaxies: ISM; Galaxies: kinematics and dynamics; Galaxies: magnetic fields; MHD; Waves

Indexed keywords

DENSITY OF GASES; GALAXIES; GASES; GRAVITATION;

AXISYMMETRIC; COMPOSITE DISC; DARK MATTER; GALAXIES: ISM; GALAXIES: KINEMATICS AND DYNAMICS; GALAXIES: MAGNETIC FIELDS; GALAXY:HALO; GRAVITATIONAL POTENTIAL; MAGNETIC-FIELD; STATIONARY PERTURBATIONS;

MAGNETOHYDRODYNAMICS;

EID: 67651119932     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2009.14965.x     Document Type: Article

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