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

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

Research output: Contribution to journalConference article

Original languageEnglish
Pages (from-to)1993-1997
JournalProc.of 28th ICRC
Publication statusPublished - 2003 Aug 1

Cite this

Yoshida, K., Y.Komori, Y. K., T.Kobayashi, T. K., & J.Nishimura, J. N. (2003). The Origin of High Energy Cosmic-Ray Electrons and Nearby Supernova Remnants. Proc.of 28th ICRC, 1993-1997.

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

In: Proc.of 28th ICRC, 01.08.2003, p. 1993-1997.

Research output: Contribution to journalConference article

Yoshida, K, Y.Komori, YK, T.Kobayashi, TK & J.Nishimura, JN 2003, 'The Origin of High Energy Cosmic-Ray Electrons and Nearby Supernova Remnants', Proc.of 28th ICRC, pp. 1993-1997.
Yoshida K, Y.Komori YK, T.Kobayashi TK, J.Nishimura JN. The Origin of High Energy Cosmic-Ray Electrons and Nearby Supernova Remnants. Proc.of 28th ICRC. 2003 Aug 1;1993-1997.
Yoshida, Kenji ; Y.Komori, Y.Komori ; T.Kobayashi, T.Kobayashi ; J.Nishimura, J.Nishimura. / The Origin of High Energy Cosmic-Ray Electrons and Nearby Supernova Remnants. In: Proc.of 28th ICRC. 2003 ; pp. 1993-1997.
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AU - J.Nishimura, J.Nishimura

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