SEUNGKYUNG  OH

skoh <at> astro.uni-bonn.de

Argelander-Institut für Astronomie
Universität Bonn
Auf dem Hügel 71
D-53121 Bonn, Germany

Tel : +49 228 73 9399


RESEARCH


Massive stars in young star clusters
Mass distribution at the central parsecs of our Galaxy (subject of Master's thesis)

Publications

"The emergence of super-canonical stars in R136-type star-burst clusters"
     S. Banerjee, P. Kroupa, S. Oh, MNRAS, 426, 1416, 2012 [ADS]

"The influence of stellar-dynamical ejections and collisions on the relation between the maximum-star and star-cluster-mass"
     S. Oh and P. Kroupa, MNRAS, 424, 65, 2012 [ADS]

"Runaway massive stars from R136: VFTS 682 is very likely a slow runaway"
     S. Banerjee, P. Kroupa, S. Oh, ApJ, 746, 15, 2012 [ADS]

"Search for OB stars running away from young star clusters. II. The NGC 6357 star-forming region"
     V. V. Gvaramadze, A. Y. Kniazev, P. Kroupa, S. Oh, A&A, 535, 29, 2011 [ADS]

"An analytical description of the evolution of binary orbital-parameter distributions in N-body computations of star clusters"
     M. Marks, P. Kroupa, S. Oh, MNRAS, 417, 1684, 2011 [ADS]

"Mass distribution in the central few parsecs of our Galaxy"
     S. Oh, S. S. Kim, D. F. Figer, JKAS, 42, 17, 2009 [ADS]

"Theoretical isochrones with extinction in the K band"
     S. S. Kim, D. F. Figer, M. G. Lee, S. Oh, PASP, 117, 445, 2005 [ADS]


BACKGROUND


2007- Ph.D. student, Argelander-Institut für Astronomie, University of Bonn, Germany
                            IMPRS, Max-Planck-Institut für Radioastronomie, Germany
2006, M.S., Dept. of Astronomy & Space Sci., Kyung Hee Univ., Korea
2004, B.S., Dept. of Astronomy & Space Sci., Kyung Hee Univ., Korea

 

Last Update: 29. Jan. 2013