An evolutionary model for pulsar-driven supernova remnants a hydrodynamical model

Astronomy and Astrophysics

Volumn 420, Issue 3, 2004, Pages 937-944

  Van Der Swaluw, E ^a,b   Downes, T P ^c   Keegan, R ^c  

^a DUBLIN INSTITUTE FOR ADVANCED STUDIES   (Ireland)

^b FOM INSTITUTE FOR PLASMA PHYSICS RIJNHUIZEN   (Netherlands)

^c DUBLIN CITY UNIVERSITY   (Ireland)

Author keywords

Hydrodynamics; Pulsars: general; Shocks waves; Stars: supernova remnants

Indexed keywords

BUBBLES (IN FLUIDS); COMPUTER SIMULATION; HYDRODYNAMICS; MATHEMATICAL MODELS; SHOCK WAVES; SIGNAL TO NOISE RATIO; WIND EFFECTS;

MECHANICAL ENERGY; PULSARS: GENERAL; STARS: SUPERNOVA REMNANTS;

ASTROPHYSICS;

EID: 3042689879     PISSN: 00046361     EISSN: None     Source Type: Journal    
DOI: 10.1051/0004-6361:20035700     Document Type: Article

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