On the self-consistent model of an axisymmetric radio pulsar magnetosphere

Monthly Notices of the Royal Astronomical Society

Volumn 298, Issue 3, 1998, Pages 847-853

  Beskin, V S ^a   Malyshkin, L M ^b,c  

^a LEBEDEV PHYSICAL INSTITUTE   (Russian Federation)

^b MOSCOW INSTITUTE OF PHYSICS AND TECHNOLOGY   (Russian Federation)

^c PRINCETON UNIVERSITY   (United States)

Author keywords

Methods: numerical; Pulsars: general; Radio continuum: general; Stars: magnetic fields; Stars: neutron

Indexed keywords

MAGNETIC FIELDS; NUMERICAL METHODS; PULSARS;

AXISYMMETRIC; MAGNETIC-FIELD; METHOD: NUMERICAL; PULSARS: GENERAL; RADIO CONTINUUM: GENERAL; RADIO PULSARS; SELF CONSISTENT MODELING; SEPARATRIX; STARS: MAGNETIC FIELD; STARS: NEUTRONS;

MAGNETOSPHERE;

EID: 0007114807     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.1998.01665.x     Document Type: Article

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