The Origin of High-Energy Cosmic-Ray Electrons and Nearby Supernova Remnants

K.Yoshida K.Yoshida, Y.Komori Y.Komori, T.Kobayashi T.Kobayashi, J.Nishimura J.Nishimura, Kenji Yoshida

Research output: Contribution to journalArticle

Original languageEnglish
JournalDefault journal
Publication statusPublished - 2003 Aug 1

Cite this

K.Yoshida, K. Y., Y.Komori, Y. K., T.Kobayashi, T. K., J.Nishimura, J. N., & Yoshida, K. (2003). The Origin of High-Energy Cosmic-Ray Electrons and Nearby Supernova Remnants. Default journal.

The Origin of High-Energy Cosmic-Ray Electrons and Nearby Supernova Remnants. / K.Yoshida, K.Yoshida; Y.Komori, Y.Komori; T.Kobayashi, T.Kobayashi; J.Nishimura, J.Nishimura; Yoshida, Kenji.

In: Default journal, 01.08.2003.

Research output: Contribution to journalArticle

K.Yoshida, KY, Y.Komori, YK, T.Kobayashi, TK, J.Nishimura, JN & Yoshida, K 2003, 'The Origin of High-Energy Cosmic-Ray Electrons and Nearby Supernova Remnants', Default journal.
K.Yoshida KY, Y.Komori YK, T.Kobayashi TK, J.Nishimura JN, Yoshida K. The Origin of High-Energy Cosmic-Ray Electrons and Nearby Supernova Remnants. Default journal. 2003 Aug 1.
K.Yoshida, K.Yoshida ; Y.Komori, Y.Komori ; T.Kobayashi, T.Kobayashi ; J.Nishimura, J.Nishimura ; Yoshida, Kenji. / The Origin of High-Energy Cosmic-Ray Electrons and Nearby Supernova Remnants. In: Default journal. 2003.
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