메뉴 건너뛰기




Volumn 408, Issue 1, 2010, Pages

Lepto-hadronic origin of γ-rays from the G54.1+0.3 pulsar wind nebula

Author keywords

Gamma rays: ISM; ISM: individual objects: G54.1+0.3; Radiation mechanisms: non thermal

Indexed keywords


EID: 79952467344     PISSN: 17453933     EISSN: None     Source Type: Journal    
DOI: 10.1111/j.1745-3933.2010.00934.x     Document Type: Letter
Times cited : (27)

References (25)
  • 1
    • 78649298938 scopus 로고    scopus 로고
    • Acciari V. A. et al., 2010, ApJ, 719, L69
    • (2010) ApJ , vol.719
    • Acciari, V.A.1
  • 10
    • 79952472196 scopus 로고    scopus 로고
    • Fermi LAT Performance
    • Fermi LAT Performance, 2007, http://www-glast.slac.stanford.edu/software/IS/glast_lat_performance.htm
    • (2007)
  • 16
    • 56849108141 scopus 로고    scopus 로고
    • Koo B.-C. et al., 2008, ApJ, 673, L147
    • (2008) ApJ , vol.673
    • Koo, B.-C.1
  • 23
    • 70549107458 scopus 로고    scopus 로고
    • Becker W., Huang H.-H., eds, MPE Rep. 291. Max Planck Institute for Extraterrestrial Physics, Garching
    • Venter C., de Jager O. C., 2006, in Becker W., Huang H.-H., eds, Proc. 363rd WE-Heraeus Seminar on Neutron Stars and Pulsars, MPE Rep. 291. Max Planck Institute for Extraterrestrial Physics, Garching, p. 40
    • (2006) Proc. 363rd WE-Heraeus Seminar on Neutron Stars and Pulsars , pp. 40
    • Venter, C.1    de Jager, O.C.2


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.