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 journalMeeting Abstract

Original languageEnglish
JournalDefault journal
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. Default journal.

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: Default journal, 01.08.2003.

Research output: Contribution to journalMeeting Abstract

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: Default journal. 2003.
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AU - J.Nishimura, J.Nishimura

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