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The Acceleration of Cosmic-ray Protons in the Supernova Remnant RX J1713.7-3946

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dc.contributor.authorEnomoto, R
dc.contributor.authorNaito, T
dc.contributor.authorTanimori, T
dc.contributor.authorYoshida, T
dc.contributor.authorYanagita, S
dc.contributor.authorMori, Masaki
dc.contributor.authorEdwards, Philip G
dc.contributor.authorAsahara, A
dc.contributor.authorBicknell, Geoffrey
dc.contributor.authorGunji, S
dc.contributor.authorHara, Shinji
dc.contributor.authorHara, T
dc.contributor.authorHayashi, Sei
dc.contributor.authorItoh, Chie
dc.contributor.authorKabuki, S
dc.contributor.authorKajino, F
dc.contributor.authorKatagiri, H
dc.contributor.authorKataoka, J
dc.contributor.authorKawachi, A
dc.contributor.authorKifune, Tadashi
dc.contributor.authorKubo, H
dc.contributor.authorKushida, J
dc.contributor.authorMaeda, S
dc.contributor.authorMaeshiro, A
dc.contributor.authorMatsubara, Y
dc.contributor.authorMizumoto, Y
dc.contributor.authorMoriya, Mie
dc.contributor.authorMuraishi, H
dc.contributor.authorMuraki, Y
dc.contributor.authorNakase, T
dc.contributor.authorNishijima, K
dc.contributor.authorOhishi, M
dc.contributor.authorOkumora, K
dc.contributor.authorPatterson, Joseph R
dc.contributor.authorSakurazawa, K
dc.contributor.authorSuzuki, R
dc.contributor.authorSwaby, D L
dc.contributor.authorTakano, K
dc.contributor.authorTakata, M
dc.contributor.authorTokanai, F
dc.contributor.authorTsuchiya, K
dc.contributor.authorTsunoo, H
dc.contributor.authorUruma, K
dc.contributor.authorWatanabe, O
dc.contributor.authorYoshikoshi, T
dc.date.accessioned2015-12-13T22:29:16Z
dc.date.issued2002
dc.date.updated2015-12-11T08:47:43Z
dc.description.abstractProtons with energies up to ∼1015 eV are the main component of cosmic rays, but evidence for the specific locations where they could have been accelerated to these energies has been lacking. Electrons are known to be accelerated to cosmic-ray energies i
dc.identifier.issn0028-0836
dc.identifier.urihttp://hdl.handle.net/1885/74615
dc.publisherMacmillan Publishers Ltd
dc.sourceNature
dc.subjectKeywords: Acceleration; Cosmic rays; Electrons; Gamma rays; Shock waves; Spectrum analysis; Upper atmosphere; Cosmic-ray protons; Protons; proton; cosmic ray; article; astronomy; cosmic radiation; electron; gamma radiation; negative pion radiation; photon; priority
dc.titleThe Acceleration of Cosmic-ray Protons in the Supernova Remnant RX J1713.7-3946
dc.typeJournal article
local.bibliographicCitation.lastpage825
local.bibliographicCitation.startpage823
local.contributor.affiliationEnomoto, R, University of Tokyo
local.contributor.affiliationNaito, T, Yamanashi Gakuin University
local.contributor.affiliationTanimori, T, Kyoto University
local.contributor.affiliationYoshida, T, Ibaraki University
local.contributor.affiliationYanagita, S, Ibaraki University
local.contributor.affiliationMori, Masaki, University of Tokyo
local.contributor.affiliationEdwards, Philip G, Japan Aerospace Exploration Agency
local.contributor.affiliationAsahara, A, Kyoto University
local.contributor.affiliationBicknell, Geoffrey, College of Physical and Mathematical Sciences, ANU
local.contributor.affiliationGunji, S, Yamagata University
local.contributor.affiliationHara, Shinji, University of Tokyo
local.contributor.affiliationHara, T, Yamanashi Gakuin University
local.contributor.affiliationHayashi, Sei, Konan University
local.contributor.affiliationItoh, Chie, Ibaraki Prefectural University of Health Sciences
local.contributor.affiliationKabuki, S, University of Tokyo
local.contributor.affiliationKajino, F, Konan University
local.contributor.affiliationKatagiri, H, University of Tokyo
local.contributor.affiliationKataoka, J, Kyoto University
local.contributor.affiliationKawachi, A, University of Tokyo
local.contributor.affiliationKifune, Tadashi, Shinshu University
local.contributor.affiliationKubo, H, Kyoto University
local.contributor.affiliationKushida, J, Tokai University
local.contributor.affiliationMaeda, S, Konan University
local.contributor.affiliationMaeshiro, A, Konan University
local.contributor.affiliationMatsubara, Y, Nagoya University
local.contributor.affiliationMizumoto, Y, National Astronomical Observatory of Japan
local.contributor.affiliationMoriya, Mie, Shinshu University
local.contributor.affiliationMuraishi, H, Kitasato University
local.contributor.affiliationMuraki, Y, Nagoya University
local.contributor.affiliationNakase, T, Tokai University
local.contributor.affiliationNishijima, K, Tokai University
local.contributor.affiliationOhishi, M, University of Tokyo
local.contributor.affiliationOkumora, K, University of Tokyo
local.contributor.affiliationPatterson, Joseph R, University of Adelaide
local.contributor.affiliationSakurazawa, K, Tokyo Institute of Technology
local.contributor.affiliationSuzuki, R, University of Tokyo
local.contributor.affiliationSwaby, D L, University of Adelaide
local.contributor.affiliationTakano, K, Tokyo Institute of Technology
local.contributor.affiliationTakata, M, Japan Science and Technology Agency
local.contributor.affiliationTokanai, F, Yamagata University
local.contributor.affiliationTsuchiya, K, University of Tokyo
local.contributor.affiliationTsunoo, H, University of Tokyo
local.contributor.affiliationUruma, K, Tokai University
local.contributor.affiliationWatanabe, O, Toyota
local.contributor.affiliationYoshikoshi, T, University of Tokyo
local.contributor.authoruidBicknell, Geoffrey, u8000061
local.description.embargo2037-12-31
local.description.notesImported from ARIES
local.description.refereedYes
local.identifier.absfor020110 - Stellar Astronomy and Planetary Systems
local.identifier.ariespublicationMigratedxPub4209
local.identifier.citationvolume416
local.identifier.doi10.1038/416823a
local.identifier.scopusID2-s2.0-0037171740
local.type.statusPublished Version

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