Inverse Compton gamma radiation of faint synchrotron X-ray nebulae around pulsars

Monthly Notices of the Royal Astronomical Society

Volumn 291, Issue 1, 1997, Pages 162-176

  Aharonian, F A ^a   Atoyan, A M ^a,b   Kifune, T ^c  

^a MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^b YEREVAN PHYSICS INSTITUTE   (Armenia)

^c UNIVERSITY OF TOKYO   (Japan)

Author keywords

Gamma rays: Theory; Pulsars: Individual: PSR B1706 44; Radiation mechanisms: Non thermal; X rays: Stars

Indexed keywords

ASTROPHYSICS; ELECTRONS; GALAXIES; GAMMA RAYS; INVERSE PROBLEMS; MAGNETIC FIELDS; OBJECT DETECTION; PHOTONS; TELLURIUM COMPOUNDS; X RAY DETECTORS;

ENERGY; GAMMA RAYS: THEORY; INVERSE COMPTON; NONTHERMAL; PHOTON FIELDS; PSR B1706-44; PULSAR: INDIVIDUAL: PSR B1706 - 44; PULSARS:INDIVIDUAL; RADIATION MECHANISMS: NONTHERMAL; X-RAY:STARS;

PULSARS;

EID: 0000398756     PISSN: 00358711     EISSN: None     Source Type: Journal    
DOI: 10.1093/mnras/291.1.162     Document Type: Article

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