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

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Date

2002

Authors

Enomoto, R
Naito, T
Tanimori, T
Yoshida, T
Yanagita, S
Mori, Masaki
Edwards, Philip G
Asahara, A
Bicknell, Geoffrey
Gunji, S

Journal Title

Journal ISSN

Volume Title

Publisher

Macmillan Publishers Ltd

Abstract

Protons 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

Description

Keywords

Keywords: 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

Citation

URI

http://hdl.handle.net/1885/74615

Collections

ANU Research Publications

Source

Nature

Type

Journal article

Book Title

Entity type

Access Statement

License Rights

DOI

10.1038/416823a

Restricted until

2037-12-31

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01_Enomoto_The_Acceleration_of_Cosmic-ray_2002.pdf (280.49 KB)

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