Gamma-ray emission expected from Kepler's supernova remnant
A&A, 452 1 (2006) 217-221
Published online: 2006-05-17
Articles citing this article
The Citing articles tool gives a list of articles citing the current article.
The citing articles come from EDP Sciences database, as well as other publishers participating in CrossRef Cited-by Linking Program. You can set up your personal account to receive an email alert each time this article is cited by a new article (see the menu on the right-hand side of the abstract page).
Cited article:
This article has been cited by the following article(s):
Hadronic versus Leptonic Origin of Gamma-Ray Emission from Supernova Remnants
Nicholas J. Corso, Rebecca Diesing and Damiano CaprioliThe Astrophysical Journal 954 (1) 1 (2023)
https://doi.org/10.3847/1538-4357/ace699
Evidence for γ-ray emission from the remnant of Kepler’s supernova based on deep H.E.S.S. observations
F. Aharonian, F. Ait Benkhali, E. O. Angüner, H. Ashkar, M. Backes, V. Barbosa Martins, R. Batzofin, Y. Becherini, D. Berge, K. Bernlöhr, M. Böttcher, C. Boisson, J. Bolmont, M. de Bony de Lavergne, M. Breuhaus, R. Brose, F. Brun, T. Bulik, T. Bylund, F. Cangemi, S. Caroff, S. Casanova, M. Cerruti, T. Chand, A. Chen, et al.Astronomy & Astrophysics 662 A65 (2022)
https://doi.org/10.1051/0004-6361/202243096
Constraining the magnetic field in GRB relativistic collisionless shocks using radio data
R. Barniol DuranMonthly Notices of the Royal Astronomical Society 442 (4) 3147 (2014)
https://doi.org/10.1093/mnras/stu1070
THE ORIGIN OF KEPLER'S SUPERNOVA REMNANT
Daniel J. Patnaude, Carles Badenes, Sangwook Park and J. Martin LamingThe Astrophysical Journal 756 (1) 6 (2012)
https://doi.org/10.1088/0004-637X/756/1/6
The imprint of a symbiotic binary progenitor on the properties of Kepler’s supernova remnant
A. Chiotellis, K. M. Schure and J. VinkAstronomy & Astrophysics 537 A139 (2012)
https://doi.org/10.1051/0004-6361/201014754
Postshock turbulence and diffusive shock acceleration in young supernova remnants
A. Marcowith and F. CasseAstronomy and Astrophysics 515 A90 (2010)
https://doi.org/10.1051/0004-6361/200913022
MULTIMESSENGER MODEL FOR THE STARBURST GALAXY M82
Elsa de Cea del Pozo, Diego F. Torres and Ana Y. Rodriguez MarreroThe Astrophysical Journal 698 (2) 1054 (2009)
https://doi.org/10.1088/0004-637X/698/2/1054
Radio emission from supernova remnants: implications for post-shock magnetic field amplification & the magnetic fields of galaxies
Todd A. Thompson, Eliot Quataert and Norman MurrayMonthly Notices of the Royal Astronomical Society 397 (3) 1410 (2009)
https://doi.org/10.1111/j.1365-2966.2009.14889.x
CANGAROO‐III Search for Gamma Rays from Kepler’s Supernova Remnant
R. Enomoto, Y. Higashi, T. Yoshida, et al.The Astrophysical Journal 683 (1) 383 (2008)
https://doi.org/10.1086/589912
Non-thermal emission from old supernova remnants
Jun Fang and Li ZhangMonthly Notices of the Royal Astronomical Society 384 (3) 1119 (2008)
https://doi.org/10.1111/j.1365-2966.2007.12766.x
HESS upper limits for Kepler's supernova remnant
F. Aharonian, A. G. Akhperjanian, U. Barres de Almeida, et al.Astronomy & Astrophysics 488 (1) 219 (2008)
https://doi.org/10.1051/0004-6361:200809401
Inverse Compton gamma-ray models for remnants of Galactic type Ia supernovae?
H. J. Völk, L. T. Ksenofontov and E. G. BerezhkoAstronomy & Astrophysics 490 (2) 515 (2008)
https://doi.org/10.1051/0004-6361:200810501
Cosmic ray acceleration by supernova shocks
E.G. BerezhkoAdvances in Space Research 41 (3) 429 (2008)
https://doi.org/10.1016/j.asr.2007.04.034