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γCygni SNR morphology viewed in the electromagnetic spectrum
Vera G. Sinitsyna, Vera Y. Sinitsyna, K. A. Balygin, S. S. Borisov, A. I. Klimov, R. M. Mirzafatikhov and N. I. Moseiko Astronomische Nachrichten 345(2-3) (2024) https://doi.org/10.1002/asna.20240008
Study of the GeV to TeV morphology of the γ Cygni SNR (G 78.2+2.1) with MAGIC and Fermi-LAT
How do supernova remnants cool? – I. Morphology, optical emission lines, and shocks
Ekaterina I Makarenko, Stefanie Walch, Seamus D Clarke, et al. Monthly Notices of the Royal Astronomical Society 523(1) 1421 (2023) https://doi.org/10.1093/mnras/stad1472
Strongly pulsed thermal X-rays from a single extended hot spot on PSR J2021+4026
Michela Rigoselli, Sandro Mereghetti, Roberto Taverna, Roberto Turolla and Davide De Grandis Astronomy & Astrophysics 646 A117 (2021) https://doi.org/10.1051/0004-6361/202039774
The gas-to-extinction ratio and the gas distribution in the Galaxy
Hui Zhu, Wenwu Tian, Aigen Li and Mengfei Zhang Monthly Notices of the Royal Astronomical Society 471(3) 3494 (2017) https://doi.org/10.1093/mnras/stx1580
THE GIGAELECTRONVOLT COUNTERPART OF VER J2019+407 IN THE NORTHERN SHELL OF THE SUPERNOVA REMNANT G78.2+2.1 (γ Cygni)
A Cocoon of Freshly Accelerated Cosmic Rays Detected by Fermi in the Cygnus Superbubble
M. Ackermann, M. Ajello, A. Allafort, L. Baldini, J. Ballet, G. Barbiellini, D. Bastieri, A. Belfiore, R. Bellazzini, B. Berenji, R. D. Blandford, E. D. Bloom, E. Bonamente, A. W. Borgland, E. Bottacini, M. Brigida, P. Bruel, R. Buehler, S. Buson, G. A. Caliandro, R. A. Cameron, P. A. Caraveo, J. M. Casandjian, C. Cecchi, A. Chekhtman, et al. Science 334(6059) 1103 (2011) https://doi.org/10.1126/science.1210311
THE IDENTIFICATION OF THE X-RAY COUNTERPART TO PSR J2021+4026