collaborators

4 papers

astro-ph.HE2026

Superlinear Type II Superluminous Supernovae 2017fck and 2019cmv: A Possible Origin from Interacting Thermonuclear Supernovae

Daichi Hiramatsu, Takashi J. Moriya, D. Andrew Howell +9

Additional power sources to traditional supernovae (SNe) are necessary to account for the extreme luminosities of superluminous SNe (SLSNe). A main power source for hydrogen-rich S…

astro-ph.HE2026

Electron-capture Supernova Candidates from Light Curves: Implications for Their Progenitors and Explosion Properties

Masato Sato, Nozomu Tominaga, Sergei I. Blinnikov +5

Core-collapse supernovae are explosions of massive stars. While most massive stars end as iron-core-collapse supernovae, less massive stars are expected to explode as electron-capt…

physics.ao-ph2025

Considerations of Earth climate sensitivity based on peculiarities of planetary heat capacity using system identification method: Runaway greenhouse effect scenario is still possible

Alexei V Karnaukhov, Sergei F Lyuksyutov, Artem V Aliakin +2

System identification method (SIM) was used to evaluate the Earth equilibrium climate sensitivity. According to our simulations, the equilibrium climate sensitivity was found to be…

astro-ph.HE2025

Type Ibn supernovae from ultra-stripped supernova progenitors

Takashi J. Moriya, Bernhard Mueller, Sergei I. Blinnikov +4

Ultra-stripped supernovae are core-collapse supernovae from progenitors that lose a significant fraction of mass because of the binary interactions with their compact companion sta…