Axially symmetric relativistic MHD simulations of pulsar wind nebulae in supernova remnants on the origin of torus and jet-like features

Astronomy and Astrophysics

Volumn 421, Issue 3, 2004, Pages 1063-1073

  Del Zanna, L ^a   Amato, E ^b   Bucciantini, N ^a  

^a UNIVERSITY OF FLORENCE   (Italy)

^b INAF OSSERVATORIO ASTROFISICO DI ARCETRI   (Italy)

Author keywords

ISM: jets and outflows; ISM: supernova remnants; Magnetohydrodynamics (MHD); Relativity; Shock waves; Stars: pulsars: general

Indexed keywords

ENERGY DISSIPATION; JETS; MAGNETIZATION; MAGNETOHYDRODYNAMICS; MATHEMATICAL MODELS; NATURAL FREQUENCIES; NUMERICAL METHODS; SHOCK WAVES; VELOCITY MEASUREMENT; X RAYS;

INTERSTELLAR MEDIUM (ISM); JETS AND OUTFLOWS; STARS:PULSARS; SUPERNOVA REMNANTS (SNR);

ASTROPHYSICS;

EID: 3142702327     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20035936     Document Type: Article

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