Please use this identifier to cite or link to this item: http://hdl.handle.net/2440/37556
Citations
Scopus Web of Science® Altmetric
?
?
Type: Journal article
Title: High-energy particle acceleration in the shell of a supernova remnant
Author: Aharonian, F.
Akhperjanian, A.
Aye, K.
Bazer-Bachi, A.
Beilicke, M.
Benbow, W.
Berge, D.
Berghaus, P.
Bernlohr, K.
Bolz, O.
Boisson, C.
Borgmeier, C.
Breitling, F.
Brown, A.
Bussons Gordo, J.
Chadwick, P.
Chitnis, V.
Chounet, L.
Cornils, R.
Costamante, L.
et al.
Citation: Nature, 2004; 432(7013):75-77
Publisher: Nature Publishing Group
Issue Date: 2004
ISSN: 0028-0836
1476-4687
Statement of
Responsibility: 
F. A. Aharonian...G. Rowell...et al.
Abstract: A significant fraction of the energy density of the interstellar medium is in the form of high-energy charged particles (cosmic rays). The origin of these particles remains uncertain. Although it is generally accepted that the only sources capable of supplying the energy required to accelerate the bulk of Galactic cosmic rays are supernova explosions, and even though the mechanism of particle acceleration in expanding supernova remnant (SNR) shocks is thought to be well understood theoretically, unequivocal evidence for the production of high-energy particles in supernova shells has proven remarkably hard to find. Here we report on observations of the SNR RX J1713.7 - 3946 (G347.3 - 0.5), which was discovered by ROSAT in the X-ray spectrum and later claimed as a source of high-energy gamma-rays of TeV energies (1 TeV = 10(12) eV). We present a TeV gamma-ray image of the SNR: the spatially resolved remnant has a shell morphology similar to that seen in X-rays, which demonstrates that very-high-energy particles are accelerated there. The energy spectrum indicates efficient acceleration of charged particles to energies beyond 100 TeV, consistent with current ideas of particle acceleration in young SNR shocks.
Description: © 2004 Nature Publishing Group
RMID: 0020063315
DOI: 10.1038/nature02960
Appears in Collections:Physics publications

Files in This Item:
There are no files associated with this item.


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.