activity
20172022
most citedNon-linear Development of Secular Gravitational Instability in Protoplanetary Disks

39 citations · 47 across the 3 of their papers we have counts for

collaborators

4 papers

astro-ph.EP20228 cited

Nonlinear Outcome of Coagulation Instability in Protoplanetary Disks II: Dust Ring Formation Mediated by Backreaction and Fragmentation

Ryosuke T. Tominaga, Hidekazu Tanaka, Hiroshi Kobayashi +1

In our previous work (Paper I), we demonstrated that coagulation instability results in dust concentration against depletion due to the radial drift and accelerates dust growth loc…

astro-ph.EP2020

Secular Gravitational Instability of Drifting Dust in Protoplanetary Disks: Formation of Dusty Rings without Significant Gas Substructures

Ryosuke T. Tominaga, Sanemichi Z. Takahashi, Shu-ichiro Inutsuka

Secular gravitational instability (GI) is one of the promising mechanisms for creating annular substructures and planetesimals in protoplanetary disks. We perform numerical simulat…

astro-ph.EP2019

Revised description of dust diffusion and a new instability creating multiple rings in protoplanetary disks

Ryosuke T. Tominaga, Sanemichi Z. Takahashi, Shu-ichiro Inutsuka

Various instabilities have been proposed as a promising mechanism to accumulate dust. Moreover, some of them are expected to lead to the multiple-ring structure formation and the p…

astro-ph.EP201739 cited

Non-linear Development of Secular Gravitational Instability in Protoplanetary Disks

Ryosuke T. Tominaga, Shu-ichiro Inutsuka, Sanemichi Z. Takahashi

We perform non-linear simulation of secular gravitational instability (GI) in protoplanetary disks that has been proposed as a mechanism of the planetesimal formation and the multi…