activity
20162020
most citedCan the Uranian Satellites Form from a Debris Disk Generated by a Giant Impact?

7 citations · 14 across the 2 of their papers we have counts for

collaborators

5 papers

astro-ph.EP20207 cited

N-body Simulations of Ring Formation Process around the Dwarf Planet Haumea

Iori Sumida, Yuya Ishizawa, Natsuki Hosono +1

Haumea is the only known trans-Neptunian object with a ring. The ring is in a position that causes a 3:1 spin-orbit resonance with the rotational period of Haumea, which has a tria…

astro-ph.EP20197 cited

Can the Uranian Satellites Form from a Debris Disk Generated by a Giant Impact?

Yuya Ishizawa, Takanori Sasaki, Natsuki Hosono

Hydrodynamic simulations of a giant impact to proto-Uranus indicated that such an impact could tilt its rotational axis and produce a circumplanetary debris disk beyond the corotat…

astro-ph.IM2018

Fortran interface layer of the framework for developing particle simulator FDPS

Daisuke Namekata, Masaki Iwasawa, Keigo Nitadori +6

Numerical simulations based on particle methods have been widely used in various fields including astrophysics. To date, simulation softwares have been developed by individual rese…

astro-ph.EP2018

Particle Number Dependence of The -Body Simulations of Moon Formation

Takanori Sasaki, Natsuki Hosono

The formation of the Moon from the circumterrestrial disk has been investigated by using -body simulations with the number of particles limited from to . We dev…

astro-ph.IM2016

A comparison of SPH artificial viscosities and their impact on the Keplerian disk

Natsuki Hosono, Takayuki R. Saitoh, Junichiro Makino

Hydrodynamical simulations of rotating disk play important roles in the field of astrophysical and planetary science. Smoothed Particle Hydrodynamics (SPH) has been widely used for…