Gamma-ray emission from pulsars: Strength of the acceleration field in the outer gap

Monthly Notices of the Royal Astronomical Society

Volumn 317, Issue 2, 2000, Pages 225-233

  Hirotani, Kouichi ^a  

^a NATIONAL ASTRONOMICAL OBSERVATORY OF JAPAN   (Japan)

Author keywords

Magnetic fields; Pulsars: individual: B0656+14; Pulsars: individual: B1055 52; Pulsars: individual: Geminga; Pulsars: individual: J0437 4715; Pulsars: individual: Vela

Indexed keywords

COSMIC RAYS; COSMOLOGY; ELECTRIC FIELDS; ELECTRIC LINES; GAMMA RAYS; GERMANIUM COMPOUNDS; MAGNETIC MOMENTS; MAGNETOSPHERE; PHOTONS; PULSARS; TELESCOPES; TELLURIUM COMPOUNDS;

MAGNETIC-FIELD; PULSAR: INDIVIDUAL: B0656+14; PULSAR: INDIVIDUAL: B1055-52; PULSAR: INDIVIDUAL: J0437-4715; PULSAR: INDIVIDUAL: VELA; PULSARS: INDIVIDUAL: GEMINGA; PULSARS:INDIVIDUAL;

MAGNETIC FIELDS;

EID: 0000686428     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1046/j.1365-8711.2000.03513.x     Document Type: Article

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