116 citations · 250 across the 4 of their papers we have counts for
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Comparative study between N-body and Fokker-Planck simulations for rotating star clusters: I. Equal-mass system
Eunhyeuk Kim, Ilsang Yoon, Hyung Mok Lee +1
We have carried out N-body simulations for rotating star clusters with equal mass and compared the results with Fokker-Planck models. These two different approaches are found to pr…
X-ray Tail in NGC 7619
Dong-Woo Kim, Eunhyeuk Kim, Giuseppina Fabbiano +1
We present new observational results of NGC 7619, an elliptical galaxy with a prominent X-ray tail and a dominant member of the Pegasus group. With Chandra and XMM-Newton observati…
2D Fokker-Planck models of rotating clusters
J. Fiestas, R. Spurzem, E. Kim
Globular clusters rotate significantly, and with the increasing amount of detailed morphologicaland kinematical data obtained in recent years on galactic globular clusters many int…
Spectroscopic Confirmation of a Large AGN Population in Clusters of Galaxies
Paul Martini, Daniel D. Kelson, Eunhyeuk Kim +2
We have completed a spectroscopic survey of X-ray point sources in eight low-redshift clusters of galaxies (0.05<z<0.31) and have identified 40 cluster members with broad-band (0.3…
Low Mass X-ray Binaries in 6 Elliptical Galaxies: Connection to Globular Clusters
Eunhyeuk Kim, Dong-Woo Kim, Giuseppina Fabbiano +4
We present a systematic study of the low mass X-ray binary (LMXB) populations of 6 elliptical galaxies. We utilize Chandra archival data to identify 665 X-ray point sources and HST…
Dynamical Evolution of Rotating Stellar Systems: III. The Effect of Mass Spectrum
Eunhyeuk Kim, Hyung Mok Lee, Rainer Spurzem
We have studied the dynamical evolution of rotating star clusters with mass spectrum using a Fokker-Planck code. As a simplest multi-mass model, we first investigated the two-compo…