Is the low-energy tail of shock-accelerated protons responsible for over-ionized plasma in supernova remnants?

Author(s):: Sawada, M.; Gu, L.; Yamazaki, R.

Published: 2024
Publication type: Article / Letter to editor

Date issued: 2024
Language: English
Is part of: Publications of Astronomical Society of Japan (2024), Vol. 76, no. 6, p. 1158-1172
hdl: 1887/4179898
doi: 10.1093/pasj/psae077
URL: https://ui.adsabs.harvard.edu/abs/2024PASJ...76.1158S