activity
20032023
most citedOn the minimum mass of neutron stars

148 citations · 3k across the 69 of their papers we have counts for

collaborators

69 papers

astro-ph.HE2023

Examining Neutrino-Matter Interactions in the Cassiopeia A Supernova

Toshiki Sato, Takashi Yoshida, Hideyuki Umeda +4

Neutrino interactions with stellar material are widely believed to be fundamental to the explosion of massive stars. However, this important process has remained difficult to confi…

astro-ph.HE2023★ 7 cited

Progenitor constraint with circumstellar material for the magnetar-hosting supernova remnant RCW 103

Takuto Narita, Hiroyuki Uchida, Takashi Yoshida +2

Stellar winds blown out from massive stars () contain precious information on the progenitor itself, and in this context, the most important elements are carbo…

astro-ph.SR2023★ 22 cited

Monotonicity of the cores of massive stars

Koh Takahashi, Tomoya Takiwaki, Takashi Yoshida

Massive stars are linked with diverse astronomical processes and objects including star formation, supernovae and their remnants, cosmic rays, interstellar media, and galaxy evolut…

astro-ph.HE2022★ 1 cited

On the population III binary black hole mergers with intermediate mass black holes: dependence on common envelope parameter

Kotaro Hijikawa, Tomoya Kinugawa, Ataru Tanikawa +2

The current gravitational wave (GW) detectors have successfully observed many binary compact objects, and the third generation ground-based GW detectors such as Einstein telescope…

astro-ph.SR2022★ 36 cited

Stability analysis of supermassive primordial stars: a new mass range for general relativistic instability supernovae

Chris Nagele, Hideyuki Umeda, Koh Takahashi +2

Observed supermassive black holes in the early universe have several proposed formation channels, in part because most of these channels are difficult to probe. One of the more pro…

astro-ph.SR2022★ 12 cited

Stellar models of Betelgeuse constrained using observed surface conditions

Tianyin Luo, Hideyuki Umeda, Takashi Yoshida +1

We study stellar models for Betelgeuse using the HR diagram and surface abundances as observational constraints. Previous studies on Betelgeuse have not systematically investigated…