activity
20172022
most citedStar cluster formation and cloud dispersal by radiative feedback: dependence on metallicity and compactness

57 citations · 193 across the 10 of their papers we have counts for

collaborators

24 papers

astro-ph.GA202216 cited

Far and extreme UV radiation feedback in molecular clouds and its influence on the mass and size of star clusters

Hajime Fukushima, Hidenobu Yajima

We study the formation of star clusters in molecular clouds by performing three-dimensional radiation hydrodynamics simulations with far ultraviolet (FUV; $6 ~{\rm eV} \leqq h ν\le…

astro-ph.GA2021

Formation of the first galaxies in the aftermath of the first supernovae

Makito Abe, Hidenobu Yajima, Sadegh Khochfar +2

We perform high-resolution cosmological hydrodynamic simulations to study the formation of the first galaxies that reach the masses of at . The resol…

astro-ph.GA2021

Radiation hydrodynamics simulations of massive star cluster formation in giant molecular clouds

Hajime Fukushima, Hidenobu Yajima

By performing three-dimensional radiation hydrodynamics simulations, we study the formation of young massive star clusters (YMCs, ) in clouds with the surface…

astro-ph.GA2021

Instability analysis for spiral arms of local galaxies: M51, NGC3627 and NGC628

Shigeki Inoue, Toshinobu Takagi, Atsushi Miyazaki +3

We investigate dynamical states of grand-design spiral arms in three local galaxies: M51, NGC3627 and NGC628. Based on linear perturbation analysis considering multiple components…

astro-ph.GA20211 cited

Capturing the inside-out quenching by black holes with far-infrared atomic line ratios

Shigeki Inoue, Hiroshi Matsuo, Naoki Yoshida +2

We propose to use relative strengths of far-infrared fine structure lines from galaxies to characterise early phases of the inside-out quenching by massive black holes (BHs). The B…

astro-ph.GA202018 cited

The Formation of the First Quasars. I. The Black Hole Seeds, Accretion and Feedback Models

Qirong Zhu, Yuexing Li, Yiting Li +4

Supermassive black holes (SMBHs) of are generally believed to be the central engines of the luminous quasars observed at , but their astrophysical…