Shin Inoue

most citedMajor merger fraction along the massive galaxy quenching channel at 0.2

< z <

0.7

2 citations · 2 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.GA2025

Cloud-cloud collisions in the Antennae galaxies: Does high-speed collision suppress star formation?

Shin Inoue, Kouji Ohta, Fumiya Maeda

Cloud-cloud collision (CCC) has been proposed as a mechanism for triggering massive star formation. Observations in the Milky Way and nearby galaxies have revealed the presence of…

astro-ph.GA2025

Galactic structure dependence of cloud-cloud collisions driven star formation in the barred galaxy NGC 3627

Fumiya Maeda, Kouji Ohta, Fumi Egusa +4

While cloud-cloud collisions (CCCs) have been proposed as a mechanism for triggering massive star formation, it is suggested that higher collision velocities ( $v_{col}$ ) and lo…

astro-ph.GA2024★ 2 cited

Major merger fraction along the massive galaxy quenching channel at 0.2 $< z <$ 0.7

Shin Inoue, Kouji Ohta, Yoshihisa Asada +4

We study the major merger fraction along the massive galaxy quenching channel (traced with rest-frame $NUV - r$ color) at $z =$ 0.2-0.7, aiming to examine the Cosmic Web Deta…

Cloud-cloud collisions in the Antennae galaxies: Does high-speed collision suppress star formation?

Galactic structure dependence of cloud-cloud collisions driven star formation in the barred galaxy NGC 3627

Major merger fraction along the massive galaxy quenching channel at 0.2<z<0.7

Major merger fraction along the massive galaxy quenching channel at 0.2 $< z <$ 0.7