activity
20182025
most citedTrans-Neptunian Objects Transiently Stuck in Neptune's Mean Motion Resonances: Numerical simulations of the current population

35 citations · 89 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.EP2025★ 1 cited

Dynamical Excitation as a probe of planetary origins

Brad M. S. Hansen, Tze-Yeung Yu, Neel Nagarajan +1

We present a set of numerical simulations of the dynamical evolution of compact planetary systems migrating in a protoplanetary disk whose inner edge is sculpted by the interaction…

astro-ph.EP2024★ 7 cited

Widespread disruption of resonant chains during protoplanetary disk dispersal

Brad M. S. Hansen, Tze-Yeung Yu, Yasuhiro Hasegawa

We describe the evolution of low mass planets in a dispersing protoplanetary disk around a Solar mass star. The disk model is based on the results of Yu, Hansen & Hasegawa (2023),…

astro-ph.EP2024★ 2 cited

Predicting the Dominant Formation Mechanism of Multi-Planetary Systems

Cheyanne Shariat, Yasuhiro Hasegawa, Bradley M. S. Hansen +2

Most, if not all, sun-like stars host one or more planets, making multi-planetary systems commonplace in our galaxy. We utilize hundreds of multi-planet simulations to explore the…

astro-ph.EP2022★ 2 cited

Halting Migration in Magnetospherically Sculpted Protoplanetary Disks

Tze Yeung Mathew Yu, Brad Hansen, Yasuhiro Hasegawa

We present a physically motivated model for the manner in which a stellar magnetic field sculpts the inner edge of a protoplanetary disk, and examine the consequence for the migrat…

astro-ph.EP2019★ 8 cited

Close-in giant-planet formation via in-situ gas accretion and their natal disk properties

Yasuhiro Hasegawa, Tze Yeung Mathew Yu, Bradley M. S. Hansen

The origin of close-in Jovian planets is still elusive. We examine the in-situ gas accretion scenario as a formation mechanism of these planets. We reconstruct natal disk propertie…

astro-ph.EP2018★ 35 cited

Trans-Neptunian Objects Transiently Stuck in Neptune's Mean Motion Resonances: Numerical simulations of the current population

Tze Yeung Mathew Yu, Ruth Murray-Clay, Kathryn Volk

A substantial fraction of our solar system's trans-Neptunian objects (TNOs) are in mean motion resonance with Neptune. Many of these objects were likely caught into resonances by p…

astro-ph.EP2018★ 34 cited

OSSOS IX: two objects in Neptune's 9:1 resonance -- implications for resonance sticking in the scattering population

Kathryn Volk, Ruth A. Murray-Clay, Brett J. Gladman +12

We discuss the detection in the Outer Solar System Origins Survey (OSSOS) of two objects in Neptune's distant 9:1 mean motion resonance at semimajor axis ~au. Both ob…