Relativistic magnetohydrodynamics winds from rotating neutron stars

Monthly Notices of the Royal Astronomical Society

Volumn 368, Issue 4, 2006, Pages 1717-1734

  Bucciantini, N ^a   Thompson, T A ^a,c   Arons, J ^a   Quataert, E ^a   Del Zanna, L ^b  

^a UNIVERSITY OF CALIFORNIA   (United States)

^b UNIVERSITY OF FLORENCE   (Italy)

^c PRINCETON UNIVERSITY   (United States)

Author keywords

Methods: numerical; MHD; Relativity; Stars: neutron; Stars: winds, outflows

Indexed keywords

ENERGY DISSIPATION; MAGNETIC FLUX; MAGNETIZATION; MAGNETOHYDRODYNAMICS; NEUTRONS; NUMERICAL METHODS; PULSARS; RELATIVITY; ROTATION RATE;

AXISYMMETRIC; HIGH MAGNETIZATION; MASS LOSS RATE; METHOD: NUMERICAL; NEUTRON STARS; RELATIVISTIC MAGNETOHYDRODYNAMICS; SPIN-DOWN; STARS: NEUTRONS; STARS: WINDS OUTFLOWS; TIME-DEPENDENT DYNAMICS;

WIND;

EID: 33744544253     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2006.10217.x     Document Type: Article

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