Modeling and simulations of supernova remnants: A short review focused on recent progress in morphological studies
Author:
Affiliation:
1. Astrophysical Big Bang Laboratory (ABBL)Cluster for Pioneering Research, RIKEN Saitama Japan
2. Interdisciplinary Theoretical and Mathematical Sciences Program (iTHEMS)RIKEN Saitama Japan
Funder
Pioneering Program of RIKEN for Evolution of Matter in the Universe
Publisher
Wiley
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.202023770
Reference51 articles.
1. A model grid for the spectral analysis of X-ray emission in young Type Ia supernova remnants
2. Nonlinear shock acceleration in the presence of seed particles
3. The origin of galactic cosmic rays
4. On the role of injection in kinetic approaches to non-linear particle acceleration at non-relativistic shock waves
5. Rayleigh‐Taylor Instabilities in Young Supernova Remnants Undergoing Efficient Particle Acceleration
Cited by 1 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. Evolutions of Young Type Ia Supernova Remnants with Two Initial Density Profiles in a Turbulent Medium;The Astrophysical Journal;2021-03-01
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