Recombining plasma in supernova remnants: Discovery and progress in the last decade
Author:
Affiliation:
1. Institute of Space and Astronautical ScienceJAXA Sagamihara Japan
2. Department of PhysicsThe University of Tokyo Tokyo Japan
Funder
Japan Society for the Promotion of Science
National Aeronautics and Space Administration
Publisher
Wiley
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.202023771
Reference49 articles.
1. Are the Models for Type Ia Supernova Progenitors Consistent with the Properties of Supernova Remnants?
2. The Transition from Young to Middle-aged Supernova Remnants: Thermal and Nonthermal Aspects of SNR N132D
3. A NEW APPROACH TO ANALYZING SOLAR CORONAL SPECTRA AND UPDATED COLLISIONAL IONIZATION EQUILIBRIUM CALCULATIONS. II. UPDATED IONIZATION RATE COEFFICIENTS
4. Modeling W44 as a Supernova Remnant in a Density Gradient with a Partially Formed Dense Shell and Thermal Conduction in the Hot Interior. I. The Analytical Model
5. RECOMBINING PLASMA IN THE GAMMA-RAY-EMITTING MIXED-MORPHOLOGY SUPERNOVA REMNANT 3C 391
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1. Thermal Processes in Supernova Remnants;Handbook of X-ray and Gamma-ray Astrophysics;2024
2. ALMA Observations of Supernova Remnant N49 in the Large Magellanic Cloud. II. Non-LTE Analysis of Shock-heated Molecular Clouds;The Astrophysical Journal;2023-11-01
3. Thermal Processes in Supernova Remnants;Handbook of X-ray and Gamma-ray Astrophysics;2022-11-29
4. Discovery of a Wind-blown Bubble Associated with the Supernova Remnant G346.6-0.2: A Hint for the Origin of Recombining Plasma;The Astrophysical Journal;2021-12-01
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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