The most likely sources of high-energy cosmic-ray electrons in supernova remnants

Astrophysical Journal

Volumn 601, Issue 1 I, 2004, Pages 340-351

  Kobayashi, T ^a   Komori, Y ^b   Yoshida, K ^c   Nishimura, J ^d  

^a AOYAMA GAKUIN UNIVERSITY   (Japan)

^b KANAGAWA UNIVERSITY OF HUMAN SERVICES   (Japan)

^c KANAGAWA UNIVERSITY   (Japan)

^d JAPAN AEROSPACE EXPLORATION AGENCY   (Japan)

Author keywords

Acceleration of particles; Cosmic rays; Gamma rays: theory; Supernova remnants

Indexed keywords

EID: 1642617894     PISSN: 0004637X     EISSN: 15384357     Source Type: Journal    
DOI: 10.1086/380431     Document Type: Article

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