Magnetohydrodynamic simulations of accretion disks around a weakly magnetized neutron star in strong gravity

Advances in Space Research

Volumn 28, Issue 2-3, 2001, Pages 505-510

  Kato, Y ^a   Hayashi, M R ^b   Miyaji, S ^a   Matsumoto, R ^a  

^a CHIBA UNIVERSITY   (Japan)

^b NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

Author keywords

[No Author keywords available]

Indexed keywords

COMPUTER SIMULATION; DISKS (MACHINE COMPONENTS); MAGNETOHYDRODYNAMICS; MAGNETOSPHERE; NEUTRONS;

ACCRETION DISKS;

SPACE RESEARCH;

SOLAR SYSTEM;

EID: 0035401953     PISSN: 02731177     EISSN: None     Source Type: Journal    
DOI: 10.1016/S0273-1177(01)00428-8     Document Type: Article

References (7)

1. Disk accretion by magnetic neutron stars
2. Jets from accreting magnetic young stellar objects. II. Mechanism Physics
3. X-ray flares and mass outflows driven by magnetic interaction between a protostar and its surrounding disk
4. Quasi-periodic oscillations in bright galactic-bulge X-ray sources
5. Pulsational instability of accretion disks and QPO's
6. Sonic-point model of kilohertz quasi-periodic brightness oscillations in low-mass X-ray binaries
7. Thick accretion disks and supercritical luminosities