Geometry of the non-thermal emission in SN 1006 - Azimuthal variations of cosmic-ray acceleration
A&A, 425 1 (2004) 121-131
Published online: 2004-09-10
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https://doi.org/10.1111/j.1365-2966.2008.14251.x
A joint spectro-imaging analysis of theXMM-Newtonand HESS observations of the supernova remnant RX J1713.7-3946
F. Acero, J. Ballet, A. Decourchelle, et al.Astronomy & Astrophysics 505 (1) 157 (2009)
https://doi.org/10.1051/0004-6361/200811556
Evidence of a Curved Synchrotron Spectrum in the Supernova Remnant SN 1006
G. E. Allen, J. C. Houck and S. J. SturnerThe Astrophysical Journal 683 (2) 773 (2008)
https://doi.org/10.1086/589628
Hadronic versus leptonic origin of the gamma-ray emission from supernova remnant RX J1713.7-3946
E. G. Berezhko and H. J. VölkAstronomy & Astrophysics 492 (3) 695 (2008)
https://doi.org/10.1051/0004-6361:200810444
Supernova Remnants at High Energy
Stephen P. ReynoldsAnnual Review of Astronomy and Astrophysics 46 (1) 89 (2008)
https://doi.org/10.1146/annurev.astro.46.060407.145237
Supernova remnants, planetary nebulae and superbubbles: Prospects for new XMM‐Newton observations
A. DecourchelleAstronomische Nachrichten 329 (2) 178 (2008)
https://doi.org/10.1002/asna.200710907
Morphological Evidence for Azimuthal Variations of the Cosmic‐Ray Ion Acceleration at the Blast Wave of SN 1006
Gamil Cassam‐Chenaï, John P. Hughes, Estela M. Reynoso, Carles Badenes and David MoffettThe Astrophysical Journal 680 (2) 1180 (2008)
https://doi.org/10.1086/588015
In which shell-type SNRs should we look for gamma-rays and neutrinos from P–P collisions?
Boaz Katz and Eli WaxmanJournal of Cosmology and Astroparticle Physics 2008 (01) 018 (2008)
https://doi.org/10.1088/1475-7516/2008/01/018