activity
20192022
most citedRadio Emission from Supernovae in the Very Early Phase: Implications for the Dynamical Mass Loss of Massive Stars

20 citations · 58 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2022★ 9 cited

Long-term evolution of non-thermal emission from Type Ia and core-collapse supernova remnants in a diversified circumstellar medium

Ryosuke Kobashi, Haruo Yasuda, Shiu-Hang Lee

The contribution of galactic supernova remnants (SNRs) to the origin of cosmic rays (CRs) is an important open question in modern astrophysics. Broadband non-thermal emission is a…

astro-ph.HE2021★ 4 cited

Resurrection of Non-thermal Emissions from Type Ib/c Supernova Remnants

Haruo Yasuda, Shiu-Hang Lee, Keiichi Maeda

Supernova remnants (SNRs) are important objects in investigating the links among supernova (SN) explosion mechanism(s), progenitor stars, and cosmic-ray acceleration. Non-thermal e…

astro-ph.HE2021★ 6 cited

Dark Age of Type II Supernova Remnants

Haruo Yasuda, Shiu-Hang Lee, Keiichi Maeda

Supernova remnants (SNRs) are important objects in terms of their connections with supernova (SN) explosion mechanism(s), progenitor stars, and cosmic-ray acceleration. Non-thermal…

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…