activity
20032008
most citedFormation of Spiral-Arm Spurs and Bound Clouds in Vertically Stratified Galactic Gas Disks

148 citations · 532 across the 6 of their papers we have counts for

collaborators

9 papers

astro-ph200856 cited

Dynamical Friction of Double Perturbers in a Gaseous Medium

Hyosun Kim, Woong-Tae Kim, F. J. Sanchez-Salcedo

In many astrophysical situations, as in the coalescence of supermassive black hole pairs at gas rich galactic nuclei, the dynamical friction experienced by an object is a combinati…

astro-ph200852 cited

Galactic Spiral Shocks with Thermal Instability

Chang-Goo Kim, Woong-Tae Kim, Eve C. Ostriker

Using one-dimensional hydrodynamic simulations including interstellar heating, cooling, and thermal conduction, we investigate nonlinear evolution of gas flow across galactic spira…

astro-ph2008105 cited

Physical Properties of Tidal Features in Interacting Disk Galaxies

Sang Hoon Oh, Woong-Tae Kim, Hyung Mok Lee +1

We explore tidal interactions of a galactic disk with Toomre parameter Q ~ 2 embedded in rigid halo/bulge with a point mass companion moving in a prescribed parabolic orbit. Tidal…

astro-ph200738 cited

Heating and Turbulence Driving by Galaxy Motions in Galaxy Clusters

Woong-Tae Kim

Using three-dimensional hydrodynamic simulations, we investigate heating and turbulence driving in an intracluster medium (ICM) by orbital motions of galaxies in a galaxy cluster.…

astro-ph2007133 cited

Dynamical Friction of a Circular-Orbit Perturber in a Gaseous Medium

Hyosun Kim, Woong-Tae Kim

We investigate the gravitational wake due to, and dynamical friction on, a perturber moving on a circular orbit in a uniform gaseous medium using a semi-analytic method. This work…

astro-ph2006148 cited

Formation of Spiral-Arm Spurs and Bound Clouds in Vertically Stratified Galactic Gas Disks

Woong-Tae Kim, Eve C. Ostriker

(Abridged) We investigate the growth of spiral-arm substructure in vertically stratified, self-gravitating, galactic gas disks, using local numerical MHD simulations. Our new model…