Outer-magnetospheric model for Vela-like pulsars: Formation of sub-GeV spectrum

Monthly Notices of the Royal Astronomical Society

Volumn 348, Issue 1, 2004, Pages 241-249

  Takata, J ^a   Shibata, S ^a   Hirotani, K ^b  

^a YAMAGATA UNIVERSITY   (Japan)

^b MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

Author keywords

Gamma rays: theory; Methods: analytical; Pulsars: general pulsars: individual: PSR B1706 44; Pulsars: individual: Vela pulsar; Radiation mechanisms: non thermal

Indexed keywords

ELECTRIC FIELDS; ELECTRIC LINES; GAMMA RAYS; GERMANIUM COMPOUNDS; MAGNETIC FIELDS; MAGNETOSPHERE; ULTRAVIOLET SPECTROSCOPY;

GAMMA RAYS: THEORY; MAGNETIC FIELD LINE; METHODS:ANALYTICAL; PSR B1706-44; PULSAR: GENERAL PULSAR: INDIVIDUAL: PSR B1706-44; PULSARS: GENERAL; PULSARS:INDIVIDUAL; RADIATION MECHANISMS: NONTHERMAL; SPECTRA'S;

PULSARS;

EID: 1142276352     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2004.07356.x     Document Type: Article

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