The gas density around SN 1006
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20077742/pdf
Reference31 articles.
1. Evidence for TeV gamma ray emission from Cassiopeia A
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3. A detailed spectral and morphological study of the gamma-ray supernova remnant RX J1713.7–3946 with HESS
4. Emission of SN 1006 produced by accelerated cosmic rays
5. A mechanism for strong shock electron heating in supernova remnants
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1. Measurement of temperature relaxation in the postshock plasma of the northwestern limb of SN 1006;Publications of the Astronomical Society of Japan;2024-06-13
2. Discovery of a Shock-compressed Magnetic Field in the Northwestern Rim of the Young Supernova Remnant RX J1713.7–3946 with X-Ray Polarimetry;The Astrophysical Journal Letters;2024-05-30
3. Indication of a fast ejecta fragment in the atomic cloud interacting with the southwestern limb of SN 1006;Astronomy & Astrophysics;2024-04
4. Magnetic Structures and Turbulence in SN 1006 Revealed with Imaging X-Ray Polarimetry;The Astrophysical Journal;2023-10-27
5. An Expanding Shell of Neutral Hydrogen Associated with SN 1006: Hints for the Single-degenerate Origin and Faint Hadronic Gamma-Rays;The Astrophysical Journal;2022-07-01
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