Hadronic γ-ray images of Sedov supernova remnants
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/419/2/1421/3119040/mnras0419-1421.pdf
Reference42 articles.
1. OBSERVATIONS OF THE YOUNG SUPERNOVA REMNANT RX J1713.7–3946 WITH THEFERMILARGE AREA TELESCOPE
2. The gas density around SN 1006
3. First detection of VHEγ-rays from SN 1006 by HESS
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1. Morphology of supernova remnants and their halos;Astronomy & Astrophysics;2021-10
2. Analytical-numerical methods of investigation of processes in the supernova remnants;Visnik Nacional'noi' academii' nauk Ukrai'ni;2020-06-20
3. The effect of cosmic ray acceleration on supernova blast wave dynamics;Monthly Notices of the Royal Astronomical Society;2018-05-30
4. Radio polarization maps of shell-type SNRs – II. Sedov models with evolution of turbulent magnetic field;Monthly Notices of the Royal Astronomical Society;2017-05-18
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