3D MHD Numerical Simulations of Polarized Emission in the Turbulent Background from Young Type Ia Supernova Remnants
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/866/i=1/a=37/pdf
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1. First detection of VHEγ-rays from SN 1006 by HESS
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1. Feedback of Efficient Shock Acceleration on Magnetic-field Structure Inside Young Type Ia Supernova Remnants;Research in Astronomy and Astrophysics;2024-06-01
2. Study of the Influence of the Background Neutral Component on the Dynamics of the Envelope in Supernova Remnants;Astronomy Letters;2021-11
3. Fermi-LAT Detection of GeV γ-Ray Emission from the Highly Asymmetric Shell Supernova Remnant SNR G317.3-0.2;The Astrophysical Journal;2021-04-01
4. Young bilateral supernova remnants evolving into a turbulent interstellar magnetic field;Monthly Notices of the Royal Astronomical Society;2020-05-11
5. MHD simulations of inward shocks in Cassiopeia A;Research in Astronomy and Astrophysics;2020-04-01
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