New perspectives on the supernova remnant G78.2+2.1
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:200810599/pdf
Reference39 articles.
1. Spatial spectral index variations in Galactic shell supernova remnants G39.2-0.3 and G41.1-0.3
2. Relativistic electron populations in Cassiopeia A
3. The acceleration of cosmic rays in shock fronts - I
4. The acceleration of cosmic rays in shock fronts - II
5. Particle acceleration by astrophysical shocks
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1. Study of the GeV to TeV morphology of the γ Cygni SNR (G 78.2+2.1) with MAGIC and Fermi-LAT;Astronomy & Astrophysics;2023-01-30
2. Exploring the region encompassing γ Cygni SNR and MAGIC J2019+408 with the GMRT at 325 and 610 MHz;Astronomy & Astrophysics;2022-04
3. Arecibo-Green Bank-LOFAR Carbon Radio Recombination Line Observations toward Cold H i Clouds;The Astrophysical Journal;2022-01-01
4. Radio Counterparts of Gamma-Ray Sources in the Cygnus Region;The Astrophysical Journal Supplement Series;2021-01-22
5. AGILE Study of the Gamma-Ray Emission from the SNR G78.2+2.1 (Gamma Cygni);The Astrophysical Journal;2019-06-13
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