activity
20122025
most citedOn the minimum mass of neutron stars

148 citations · 1.6k across the 38 of their papers we have counts for

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Showing 2019Show all

5 papers · 1 filter

astro-ph.HE2019★ 60 cited

Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Simulations with Single Star and Binary Merger Progenitor Models for SN 1987A

Masaomi Ono, Shigehiro Nagataki, Gilles Ferrand +5

We perform three-dimensional hydrodynamic simulations of aspherical core-collapse supernovae focusing on the matter mixing in SN 1987A. The impacts of four progenitor (pre-supernov…

astro-ph.SR2019★ 82 cited

The possible role of stellar mergers for the formation of multiple stellar populations in globular clusters

Long Wang, Pavel Kroupa, Koh Takahashi +1

Many possible scenarios for the formation of multiple stellar populations (MSP) in globular clusters (GCs) have been discussed so far, including the involvement of asymptotic giant…

astro-ph.HE2019★ 53 cited

Fitting formulae for evolution tracks of massive stars under extreme metal poor environments for population synthesis calculations and star cluster simulations

Ataru Tanikawa, Takashi Yoshida, Tomoya Kinugawa +2

We have devised fitting formulae for evolution tracks of massive stars with under extreme metal poor (EMP) environments for $\log (Z/Z_\odot) =…

astro-ph.SR2019★ 94 cited

One-, Two-, and Three-dimensional Simulations of Oxygen Shell Burning Just Before the Core-Collapse of Massive Stars

Takashi Yoshida, Tomoya Takiwaki, Kei Kotake +3

We perform two- (2D) and three-dimensional (3D) hydrodynamics simulations of convective oxygen shell-burning that takes place deep inside a massive progenitor star of a core-collap…

astro-ph.HE2019★ 1 cited

Gravitational waves from very massive stars collapsing to a black hole

Haruki Uchida, Masaru Shibata, Koh Takahashi +1

We compute gravitational waves emitted by the collapse of a rotating very massive star (VMS) core leading directly to a black hole in axisymmetric numerical-relativity simulations.…