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Volumn 547, Issue , 2012, Pages

Cold ultrarelativistic pulsar winds as potential sources of galactic gamma-ray lines above 100 GeV

Author keywords

Gamma rays: diffuse background; Methods: analytical; Pulsars: general; Radiation mechanisms: non thermal

Indexed keywords

ALTERNATIVE SOURCE; ASTROPHYSICAL OBJECTS; ATMOSPHERIC CHERENKOV TELESCOPES; COMPTONIZATION; DARK MATTER; DIFFUSE BACKGROUND; ENERGY INTERVAL; GALACTIC PLANE; GAMMA-RAY LINE; HOTSPOTS; LINE EMISSIONS; METHODS:ANALYTICAL; PHOTON STATISTICS; POTENTIAL SOURCES; PULSARS: GENERAL; RADIATION MECHANISMS: NONTHERMAL; SPATIAL STRUCTURE; SPECTRAL FEATURE; SPECTRAL LINE;

EID: 84868624131     PISSN: 00046361     EISSN: 14320746     Source Type: Journal    
DOI: 10.1051/0004-6361/201220092     Document Type: Article
Times cited : (26)

References (25)
  • 10
    • 84868627355 scopus 로고    scopus 로고
    • Boyarsky, A., Malyshev, D., & Ruchayskiy, O. 2012 [arXiv:1205.4700]
    • Boyarsky, A., Malyshev, D., & Ruchayskiy, O. 2012 [arXiv:1205.4700]
  • 21
    • 84868614470 scopus 로고    scopus 로고
    • Su, M., & Finkbeiner, D. P. 2012 [arXiv:1207.7060]
    • Su, M., & Finkbeiner, D. P. 2012 [arXiv:1207.7060]
  • 24
    • 80053611264 scopus 로고    scopus 로고
    • VERITAS Collaboration
    • VERITAS Collaboration, Aliu, E., Arlen, T., et al. 2011, Science, 334, 69
    • (2011) Science , vol.334 , pp. 69
    • Aliu, E.1    Arlen, T.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.