no code implementations • 11 Feb 2021 • D. M. -A. Meyer, M. Pohl, M. Petrov, L. Oskinova
Our models are qualitatively consistent with the radio appearance of several remnants of high-mass progenitors, namely the bilateral G296. 5+10. 0 and the shell-type remnants CTB109 and Kes 17, respectively.
High Energy Astrophysical Phenomena Astrophysics of Galaxies Solar and Stellar Astrophysics
