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astro-ph.HE2019★ 20 cited
Radio Emission from Supernovae in the Very Early Phase: Implications for the Dynamical Mass Loss of Massive Stars
Tomoki Matsuoka, Keiichi Maeda, Shiu-Hang Lee +1
Recent high-cadence transient surveys and rapid follow-up observations indicate that some massive stars may dynamically lose their own mass within decades before supernovae (SNe).…
astro-ph.HE2019★ 19 cited
Time evolution of broadband non-thermal emission from supernova remnants in different circumstellar environments
Haruo Yasuda, Shiu-Hang Lee
Supernova remnants (SNRs) are thought to be one of the major acceleration sites of galactic cosmic rays (CRs) and an important class of objects for high-energy astrophysics. SNRs p…