The effect of the infrared excess from the Be star on inverse Compton gamma-ray production in PSR B1259-63/SS 2883

Monthly Notices of the Royal Astronomical Society

Volumn 412, Issue 3, 2011, Pages 1721-1729

  Van Soelen, B ^a   Meintjes, P J ^a  

^a UNIVERSITY OF THE FREE STATE   (South Africa)

Author keywords

Pulsars: individual: PSR B1259 63; Radiation mechanisms: non thermal; X rays: binaries

Indexed keywords

GERMANIUM COMPOUNDS; INVERSE PROBLEMS; PHOTONS; PULSARS; SHOCK WAVES; TELLURIUM COMPOUNDS;

BE STARS; BINARY SYSTEMS; GAMMA-RAYS; INFRARED EMISSIONS; INVERSE COMPTON; PULSAR: INDIVIDUAL: PSR B1259-63; PULSARS:INDIVIDUAL; RADIATION MECHANISMS: NONTHERMAL; TEV GAMMA-RAY EMISSION; X-RAYS: BINARIES;

GAMMA RAY PRODUCTION;

EID: 79953304477     PISSN: 00358711     EISSN: 13652966     Source Type: Journal    
DOI: 10.1111/j.1365-2966.2010.18008.x     Document Type: Article

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