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Volumn 399, Issue 1, 2009, Pages 157-165
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Predicted γ-ray image of SN 1006 due to inverse Compton emission
c
Consorzio COMETA
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(Italy)
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Author keywords
Acceleration of particles; ISM: cosmic rays; ISM: individual: SN 1006; ISM: supernova remnants; Radiation mechanisms: non thermal; Shock waves
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Indexed keywords
COSMIC RAYS;
COSMOLOGY;
GAMMA RAYS;
INTEGRATED CIRCUITS;
INVERSE PROBLEMS;
SPECTRUM ANALYSIS;
SUPERNOVAE;
ACCELERATION OF PARTICLES;
HIGH ENERGY STEREOSCOPIC SYSTEMS;
INVERSE COMPTON;
ISM: COSMIC RAYS;
ISM: INDIVIDUAL: SN 1006;
ISM: INDIVIDUALS;
ISM: SUPERNOVA REMNANTS;
RADIATION MECHANISMS: NONTHERMAL;
SHOCK-WAVES;
SUPERNOVA REMNANTS;
SHOCK WAVES;
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EID: 70349678610
PISSN: 00358711
EISSN: 13652966
Source Type: Journal
DOI: 10.1111/j.1365-2966.2009.15352.x Document Type: Article |
Times cited : (20)
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References (35)
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