activity
20032020
most citedMass Estimates of a Giant Planet in a Protoplanetary Disk from the Gap Structures

210 citations · 304 across the 3 of their papers we have counts for

collaborators

11 papers

astro-ph.EP2020

Accretion Properties of PDS 70b with MUSE

Jun Hashimoto, Yuhiko Aoyama, Mihoko Konishi +4

We report a new evaluation of the accretion properties of PDS~70b obtained with VLT/MUSE. The main difference from previous studies in Haffert et al. (2019) and Aoyama & Ikoma (201…

astro-ph.EP2019

Final Masses of Giant Planets III: Effect of Photoevaporation and a New Planetary Migration Model

Hidekazu Tanaka, Kiyoka Murase, Takayuki Tanigawa

We herein develop a new simple model for giant planet formation, which predicts the final mass of a giant planet born in a given disk, by adding the disk mass loss due to photoevap…

astro-ph.EP2018

Impacts of dust feedback on a dust ring induced by a planet in a protoplanetary disk

Kazuhiro D. Kanagawa, Takayuki Muto, Satoshi Okuzumi +3

When a planet forms a deep gap in a protoplanetary disk, dust grains cannot pass through the gap. As a consequence, the density of the dust grains can increase up to the same level…

astro-ph.EP2018

Theoretical Model of Hydrogen Line Emission from Accreting Gas Giants

Yuhiko Aoyama, Masahiro Ikoma, Takayuki Tanigawa

Progress in understanding of giant planet formation has been hampered by a lack of observational constraints to growing protoplanets. Recently, detection of an Hα-emission excess v…

astro-ph.EP2018

Slowing Down Type II Migration of Gas Giants to Match Observational Data

Shigeru Ida, Hidekazu Tanaka, Anders Johansen +2

The mass and semimajor axis distribution of gas giants in exoplanetary systems obtained by radial velocity surveys shows that super-jupiter-mass planets are piled up at > 1 au, whi…

astro-ph.EP2018

Suppression of atmospheric recycling of planets embedded in a protoplanetary disc by buoyancy barrier

Hiroyuki Kurokawa, Takayuki Tanigawa

The ubiquity of super-Earths poses a problem for planet formation theory to explain how they avoided becoming gas giants. Rapid recycling of the envelope gas of planets embedded in…