Self-similar solutions of viscous-resistive advection-dominated accretion flows with poloidal magnetic fields

Monthly Notices of the Royal Astronomical Society

Volumn 381, Issue 1, 2007, Pages 159-170

  Ghanbari, Jamshid ^a,b,c   Salehi, Fatemeh ^c   Abbassi, Shahram ^d  

^a FERDOWSI UNIVERSITY OF MASHHAD   (Iran)

^b SAN FRANCISCO STATE UNIVERSITY   (United States)

^c Ferdowsi University of Mashhad   (Iran)

^d DAMGHAN UNIVERSITY   (Iran)

Author keywords

Accretion, accretion discs; Magnetic fields; MHD

Indexed keywords

ADVECTION; ENERGY DISSIPATION; STARS; VISCOSITY;

ACCRETION FLOW; ACCRETION: ACCRETION DISKS; ADVECTION-DOMINATED ACCRETION FLOWS; AXISYMMETRIC; COMPACT OBJECTS; DOMINANT MECHANISM; MAGNETIC DIFFUSIVITY; MAGNETIC-FIELD; POLOIDAL MAGNETIC FIELD; SELF-SIMILAR SOLUTION;

MAGNETOHYDRODYNAMICS;

EID: 35148838096     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2007.12216.x     Document Type: Article

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