activity
20212025
most citedDust coagulation and fragmentation in a collapsing cloud core and their influence on non-ideal magnetohydrodynamic effects

21 citations · 60 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.EP2025

Impact of MHD disk wind on early evolutionary stage of protoplanetary disk and dust growth

Yoshihiro Kawasaki, Masahiro N. Machida

We perform one-dimensional protoplanetary disk evolution calculations to investigate the impact of the magnetohydrodynamic (MHD) disk wind on disk evolution and dust particle growt…

astro-ph.SR2023

Ring Gap Structure around Class I Protostar WL 17

Ayumu Shoshi, Naoto Harada, Kazuki Tokuda +7

WL 17 is a Class I object and was considered to have a ring-hole structure. We analyzed the structure around WL 17 to investigate the detailed properties of WL 17. We used ALMA arc…

astro-ph.GA2023★ 12 cited

Impact of turbulence intensity and fragmentation velocity on dust particle size evolution and non-ideal magnetohydrodynamics effects

Yoshihiro Kawasaki, Masahiro N. Machida

We investigate the influence of dust particle size evolution on non-ideal magnetohydrodynamic effects during the collapsing phase of star-forming cores, taking both the turbulence…

astro-ph.GA2022★ 14 cited

Implementation of dust particles in three-dimensional magnetohydrodynamics simulation: Dust dynamics in a collapsing cloud core

Shunta Koga, Yoshihiro Kawasaki, Masahiro N. Machida

The aim of this study is to examine dust dynamics on a large scale and investigate the coupling of dust with gas fluid in the star formation process. We propose a method for calcul…

astro-ph.SR2022★ 21 cited

Dust coagulation and fragmentation in a collapsing cloud core and their influence on non-ideal magnetohydrodynamic effects

Yoshihiro Kawasaki, Shunta Koga, Masahiro N. Machida

We determine the time evolution of the dust particle size distribution during the collapse of a cloud core, accounting for both dust coagulation and dust fragmentation, to investig…

astro-ph.SR2021★ 13 cited

Growth of Magnetorotational Instability in Circumstellar Disks around Class 0 Protostars

Yoshihiro Kawasaki, Shunta Koga, Masahiro N. Machida

We investigate the possibility of the growth of magnetorotational instability (MRI) in disks around Class 0 protostars. We construct a disk model and calculate the chemical reactio…