activity
20092023
most citedPossible Transit Timing Variations of the TrES-3 Planetary System

47 citations · 119 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.GA2023★ 9 cited

Five methods for determining pattern speeds in galaxies

Daniel Pfenniger, Kanak Saha, Yu-Ting Wu

Aims. New or refined methods for determining instantaneous scalar and vector pattern speeds from a restricted domain are developed, for applications in N-body simulations or in gal…

astro-ph.GA2021★ 1 cited

The Effect of Impact Parameters on the Formation of Massive Black Hole Binaries in Galactic Mergers

Yu-Heng Ho, Ing-Guey Jiang, Yu-Ting Wu

By employing N-body simulations, we inestigate the formation of massive black hole binaries (MBHBs) through the sinking of two massive black holes (MBHs) during galaxy mergers. Wit…

astro-ph.GA2021★ 10 cited

Morphological and Kinematical Analysis of the Double-barred Galaxy NGC 3504 Using ALMA CO (2-1) Data

Yu-Ting Wu, Alfonso Trejo, Daniel Espada +1

We present results obtained from ALMA CO (2-1) data of the double-barred galaxy NGC 3504. With three times higher angular resolution (~ 0."8) than previous studies, our observation…

astro-ph.GA2018★ 10 cited

Time-dependent Pattern Speeds in Barred Galaxies

Yu-Ting Wu, Daniel Pfenniger, Ronald E. Taam

Based on a high quality -body simulation of a double bar galaxy model, we investigate the evolution of the bar properties, including their size, strength and instantaneous patte…

astro-ph.GA2016★ 16 cited

Time-dependent Corotation Resonance in Barred Galaxies

Yu-Ting Wu, Daniel Pfenniger, Ronald E. Taam

The effective potential neighboring the corotation resonance region in barred galaxies is shown to be strongly time-dependent in any rotating frame because of the competition of ne…

astro-ph.GA2015★ 10 cited

On the Formation of Elliptical Rings in Disk Galaxies

Yu-Ting Wu, Ing-Guey Jiang

N-body simulations of galactic collisions are employed to investigate the formation of elliptical rings in disk galaxies. The relative inclination between disk and dwarf galaxies i…