Recombining Plasma and Gamma-Ray Emission in the Mixed-morphology Supernova Remnant 3C 400.2
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/842/i=1/a=22/pdf
Reference57 articles.
1. FERMI LAT DISCOVERY OF EXTENDED GAMMA-RAY EMISSION IN THE DIRECTION OF SUPERNOVA REMNANT W51C
2. OBSERVATION OF SUPERNOVA REMNANT IC 443 WITH THE FERMI LARGE AREA TELESCOPE
3. FERMILARGE AREA TELESCOPE OBSERVATIONS OF THE SUPERNOVA REMNANT W28 (G6.4–0.1)
4. Gamma-Ray Emission from the Shell of Supernova Remnant W44 Revealed by the Fermi LAT
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1. Plasma diagnostics of supernova remnant 3C 400.2 by Suzaku observations;Publications of the Astronomical Society of Japan;2024-09-11
2. Detection of a new molecular cloud in the LHAASO J2108+5157 region supporting a hadronic PeVatron scenario;Publications of the Astronomical Society of Japan;2023-04-12
3. On the Formation of Over-ionized Plasma in Evolved Supernova Remnants;The Astrophysical Journal;2022-10-01
4. Long-term Evolution of Nonthermal Emission from Type Ia and Core-collapse Supernova Remnants in a Diversified Circumstellar Medium;The Astrophysical Journal;2022-08-26
5. ALMA CO Observations of the Mixed-morphology Supernova Remnant W49B: Efficient Production of Recombining Plasma and Hadronic Gamma Rays via Shock–Cloud Interactions;The Astrophysical Journal;2021-10-01
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