Modelling the interaction between relativistic and non-relativistic winds in the binary system PSR B1259-63/SS2883*- II. Impact of the magnetization and anisotropy of the pulsar wind

Monthly Notices of the Royal Astronomical Society

Volumn 419, Issue 4, 2012, Pages 3426-3432

  Bogovalov, S V ^a   Khangulyan, D ^b   Koldoba, A V ^c   Ustyugova, G V ^c   Aharonian, F A ^d,e  

^a NATIONAL RESEARCH NUCLEAR UNIVERSITY MEPHI   (Russian Federation)

^b JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

^c KELDYSH INSTITUTE OF APPLIED MATHEMATICS   (Russian Federation)

^d DUBLIN INSTITUTE FOR ADVANCED STUDIES   (Ireland)

^e MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

Author keywords

Hydrodynamics; MHD; Pulsars: general; Shock waves

Indexed keywords

KINETIC ENERGY; KINETICS; MAGNETIZATION; MAGNETOHYDRODYNAMICS; MAGNETOPLASMA; PULSARS; SYSTEMS (METALLURGICAL); WIND;

AXISYMMETRIC; BINARY SYSTEMS; ISOTROPICS; MAGNETIC-FIELD; OPTICAL-; PROPERTY; PULSARS: GENERAL; RELATIVISTICS; ROTATION AXES; SHOCK-WAVES;

SHOCK WAVES;

EID: 84855591695     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2011.19983.x     Document Type: Article

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