Sawada, M., Gu, L., & Yamazaki, R. (2024). Is the low-energy tail of shock-accelerated protons responsible for over-ionized plasma in supernova remnants?
Chicago Style (17th ed.) CitationSawada, Makoto, Liyi Gu, and Ryo Yamazaki. Is the Low-energy Tail of Shock-accelerated Protons Responsible for Over-ionized Plasma in Supernova Remnants? 2024.
MLA (9th ed.) CitationSawada, Makoto, et al. Is the Low-energy Tail of Shock-accelerated Protons Responsible for Over-ionized Plasma in Supernova Remnants? 2024.
Warning: These citations may not always be 100% accurate.