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

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

Research output: Contribution to journalArticle

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