The Most Likely Sources of High -Energy Cosmic-Ray Electrons in Supernova Remnants

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

Research output: Contribution to journalArticle

217 Citations (Scopus)
Original languageEnglish
Pages (from-to)340-351
JournalAstrophys.J
Volume601
Publication statusPublished - 2004 Jan 1

Cite this

T.Kobayashi, T. K., Y.Komori, Y. K., K.Yoshida, K. Y., J.Nishimura, J. N., & Yoshida, K. (2004). The Most Likely Sources of High -Energy Cosmic-Ray Electrons in Supernova Remnants. Astrophys.J, 601, 340-351.

The Most Likely Sources of High -Energy Cosmic-Ray Electrons in Supernova Remnants. / T.Kobayashi, T.Kobayashi; Y.Komori, Y.Komori; K.Yoshida, K.Yoshida; J.Nishimura, J.Nishimura; Yoshida, Kenji.

In: Astrophys.J, Vol. 601, 01.01.2004, p. 340-351.

Research output: Contribution to journalArticle

T.Kobayashi, TK, Y.Komori, YK, K.Yoshida, KY, J.Nishimura, JN & Yoshida, K 2004, 'The Most Likely Sources of High -Energy Cosmic-Ray Electrons in Supernova Remnants', Astrophys.J, vol. 601, pp. 340-351.
T.Kobayashi TK, Y.Komori YK, K.Yoshida KY, J.Nishimura JN, Yoshida K. The Most Likely Sources of High -Energy Cosmic-Ray Electrons in Supernova Remnants. Astrophys.J. 2004 Jan 1;601:340-351.
T.Kobayashi, T.Kobayashi ; Y.Komori, Y.Komori ; K.Yoshida, K.Yoshida ; J.Nishimura, J.Nishimura ; Yoshida, Kenji. / The Most Likely Sources of High -Energy Cosmic-Ray Electrons in Supernova Remnants. In: Astrophys.J. 2004 ; Vol. 601. pp. 340-351.
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