activity
20022026
most citedFormation of Hot Planets by a combination of planet scattering, tidal circularization, and Kozai mechanism

537 citations · 1.6k across the 24 of their papers we have counts for

collaborators

24 papers

astro-ph.EP2026

The dust-rich, gas-depleted protosolar disk as the birthplace of chondrules

Sota Arakawa, Hidekazu Tanaka, Toshihiko Kadono +3

Chondrules are the primary components of primitive meteorites known as chondrites, and understanding their formation and accumulation is essential for elucidating the history of pl…

astro-ph.EP2022★ 3 cited

A Trio of Giant Planets Orbiting Evolved Star HD 184010

Huan-Yu Teng, Bun'ei Sato, Takuya Takarada +11

We report the discovery of a triple-giant-planet system around an evolved star HD 184010 (HR 7421, HIP 96016). This discovery is based on observations from Okayama Planet Search Pr…

astro-ph.EP2021★ 4 cited

Planet-planet scattering in presence of a companion star

Francesco Marzari, Makiko Nagasawa, Krzyszof Goździewski

Planet Planet scattering is a leading dynamical mechanism invoked to explain the present orbital distribution of exoplanets. Many stars belong to binary systems, therefore it is im…

astro-ph.EP2020★ 7 cited

Secular evolution of close in planets: the effects of general relativity

Francesco Marzari, Makiko Nagasawa

Pairs of planets in a system may end up close to their host star on eccentric orbits as a consequence of planet planet scattering, Kozai or secular migration. In this scenario, gen…

astro-ph.EP2019★ 10 cited

The influence of general-relativity effects, dynamical tides and collisions on planet-planet scattering close to the star

F. Marzari, M. Nagasawa

Planet--Planet scattering is an efficient and robust dynamical mechanism for producing eccentric exoplanets. Coupled to tidal interactions with the central star, it can also explai…

astro-ph.EP2018

Shock-Generating Planetesimals Perturbed by a Giant Planet in a Gas Disk

M. Nagasawa, K. K. Tanaka, H. Tanaka +3

We examined the excitations of planetesimals caused by the resonances of a giant planet in a protoplanetary gas disk. The highly excited planetesimals generate bow shocks, the mech…