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Volumn 526, Issue 16, 2011, Pages

Effects of non-uniform interstellar magnetic field on synchrotron X-ray and inverse-Compton γ -ray morphology of supernova remnants

Author keywords

gamma rays: ISM; ISM: supernova remnants; magnetohydrodynamics (MHD); radiation mechanisms: non thermal; shock waves; X rays: ISM

Indexed keywords

ACCURATE ANALYSIS; APPROXIMATE TREATMENT; BACK REACTION; COMPTON; DEGREE OF ASYMMETRY; ENERGY BAND; GALACTIC COSMIC RAYS; HARD X RAY; INTERSTELLAR MAGNETIC FIELDS; INTERSTELLAR MEDIUMS; INVERSE COMPTON; ISM: SUPERNOVA REMNANTS; LINE-OF-SIGHT; MAGNETIC FIELD AMPLIFICATION; MAGNETIC FIELD STRENGTHS; MAGNETOHYDRODYNAMICS (MHD); MHD SIMULATION; NONTHERMAL; NONUNIFORM; NUMERICAL CODE; RADIATION MECHANISMS: NON-THERMAL; RELATIVISTIC ELECTRON; SUPERNOVA REMNANTS; SYNCHROTRON X RAYS; SYNTHESIS CODE; THEORETICAL MODELING; X RAYS: ISM;

EID: 78651307001     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201015505     Document Type: Article
Times cited : (33)

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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.