Disc structure around strongly magnetic accretors: A full disc solution with buoyancy diffusivity

Monthly Notices of the Royal Astronomical Society

Volumn 301, Issue 2, 1998, Pages 558-568

  Campbell, C G ^a   Heptinstall, P M ^a  

^a NEWCASTLE UNIVERSITY   (United Kingdom)

Author keywords

Accretion, accretion discs; Diffusion; Magnetic fields; Stars: magnetic fields; Stars: neutron

Indexed keywords

BUOYANCY; DIFFUSION; ELECTRON SCATTERING; STARS;

ACCRETION DISCS; ACCRETION: ACCRETION DISKS; DISC STRUCTURES; FULL DISKS; FULL NUMERICAL SOLUTION; MAGNETIC BUOYANCY; MAGNETIC-FIELD; STARS: MAGNETIC FIELD; STARS: NEUTRONS; TURBULENT DIFFUSION;

MAGNETIC FIELDS;

EID: 0041578173     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.02044.x     Document Type: Article

References (5)

1. Campbell C. G., 1992, Geophys. Astrophys. Fluid. Dyn., 63, 179
2. Campbell C. G., 1997, Magnetohydrodynamics in Binary Stars. Kluwer, Dordrecht
3. Campbell C. G., 1998, MNRAS, 301, 754
4. Campbell C. G., Heptinstall P. M., 1998, MNRAS, 299, 31
5. Heptinstall P. M., 1997, PhD thesis, University of Newcastle upon Tyne