Does the inverse Compton mechanism alone explain the GeV/TeV gamma-ray emission from the Crab Nebula?

Astroparticle Physics

Volumn 3, Issue 3, 1995, Pages 275-282

  Aharonian, F A ^a   Atoyan, A M ^a,b  

^a MAX PLANCK INSTITUT FÜR KERNPHYSIK   (Germany)

^b YEREVAN PHYSICS INSTITUTE   (Armenia)

Author keywords

[No Author keywords available]

Indexed keywords

EID: 0037725635     PISSN: 09276505     EISSN: None     Source Type: Journal    
DOI: 10.1016/0927-6505(95)00006-3     Document Type: Article

References (26)

1. Confinement of the Crab pulsar's wind by its supernova remnant
2. Magnetohydrodynamic model of Crab nebula radiation
3. Particle Acceleration in Cosmic Plasmas
4. Observations of the Crab pulsar and nebula by the EGRET telescope on the Compton Gamma-Ray Observatory
5. Production of Cosmic Gamma Rays by Compton Scattering in Discrete Sources
6. Far-infrared observations of the Crab nebula
7. Recent Developments Concerning the Crab Nebula
8. The Structure of the Crab Nebula at 2{middle dot}7 and 5 GHz -- I THE OBSERVATIONS
9. A study of the Crab Nebula at 2.7 GHz with an angular resolution 3.7 x 10 arcsec - I. The observations
10. A study of the Crab Nebula - II. Radio emission from the filaments
11. Filamentary structure in Crab-like supernova remnants