Modelling interaction of relativistic and non-relativistic winds in binary system PSR B1259-63/SS2883 - I. Hydrodynamical limit

Monthly Notices of the Royal Astronomical Society

Volumn 387, Issue 1, 2008, Pages 63-72

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

^a NATIONAL RESEARCH NUCLEAR UNIVERSITY MEPHI   (Russian Federation)

^b MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^c INSTITUTE OF MATHEMATICAL MODELING   (Russian Federation)

^d KELDYSH INSTITUTE OF APPLIED MATHEMATICS   (Russian Federation)

^e DUBLIN INSTITUTE FOR ADVANCED STUDIES   (Ireland)

Author keywords

Binaries: close; Hydrodynamics; Methods: numerical; Pulsars: general; Pulsars: individual: PSR B1259 63; Shock waves

Indexed keywords

GAMMA RAYS; HYDRODYNAMICS; NUMERICAL METHODS; SHOCK WAVES; SYSTEMS (METALLURGICAL);

BINARIES: CLOSE; BINARY SYSTEMS; METHOD: NUMERICAL; MODEL INTERACTION; PULSAR: INDIVIDUAL: PSR B1259-63; PULSARS: GENERAL; PULSARS:INDIVIDUAL; RELATIVISTICS; SHOCK-WAVES; STELLAR WIND;

PULSARS;

EID: 44649085735     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2008.13226.x     Document Type: Article

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