activity
20172022
most citedKinematic modelling of clusters with Gaia: the Death Throes of the Hyades

35 citations · 81 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.GA202217 cited

Mass Segregation in the Hyades Cluster

N. Wyn Evans, Semyeong Oh

Using the Gaia colour-magnitude diagram, we assign masses to a catalogue of 979 confirmed members of the Hyades cluster and tails. By fitting the cumulative mass profile, stars wit…

astro-ph.SR202035 cited

Kinematic modelling of clusters with Gaia: the Death Throes of the Hyades

Semyeong Oh, N. Wyn Evans

The precision of the Gaia data offers a unique opportunity to study the internal velocity field of star clusters. We develop and validate a forward-modelling method for the interna…

astro-ph.SR2020

Unresolved stellar companions with Gaia DR2 astrometry

Vasily Belokurov, Zephyr Penoyre, Semyeong Oh +9

For stars with unresolved companions, motions of the centre of light and that of mass decouple, causing a single-source astrometric model to perform poorly. We show that such stars…

astro-ph.SR2019

LRP2020: The Opportunity of Young Nearby Associations with the Advent of the Gaia Mission

Jonathan Gagné, Joel Kastner, Semyeong Oh +12

This white paper proposes leveraging high-quality Gaia data available to the worldwide scientific community and complement it with support from Canadian-related facilities to place…

astro-ph.GA201921 cited

Spectroscopy of the Young Stellar Association Price-Whelan 1: Origin in the Magellanic Leading Arm and Constraints on the Milky Way Hot Halo

David L. Nidever, Adrian M. Price-Whelan, Yumi Choi +7

We report spectroscopic measurements of stars in the recently discovered young stellar association Price-Whelan 1 (PW 1), which was found in the vicinity of the Leading Arm (LA) of…

astro-ph.SR20178 cited

Spectroscopic confirmation of very-wide stellar binaries and large-separation comoving pairs from Gaia DR1

Adrian M. Price-Whelan, Semyeong Oh, David N. Spergel

Members of widely-separated stellar binaries (> 0.1 pc) or loosely bound stellar associations and clusters are born with small spreads in kinematics and chemistry, but disrupt and…