1 |
Takahashi K., &; Lee, H. M. 2000, Evolution of multimass elobular clusters in the Galactic tidal field with the effects of velocity amsotropy, MNRAS, 316, 671
DOI
ScienceOn
|
2 |
Takahashi K., & Portgies Zwart, 1998, The disruption of globular star clusters in the Galaxy: A comparative analysis between Fokker-Planck and N-body models, ApJ, 503, L49
DOI
ScienceOn
|
3 |
Weinbere, M. D. 1994, Adiabatic invariants in stellar dy-namics. 2: Gravitational shocking, AJ, 108, 1403
DOI
|
4 |
Kim, Y. K., & Oh, K. S. 1999, Dynamical evolution of the multi-mass component globular clusters under the tidal interaction with the Galaxy, JKAS, 32, 17
|
5 |
Kim, S. S., Morris M., & Lee, H. M. 1999, ApJ, Evaporation of compact young clusters near the Galactic Center, 525, 228
DOI
|
6 |
Lee, H. M., &: Goodman, J., 1995, Influence of the stellar mass function of the evaporation rate of tidally limited postcollapse globular clusters, ApJ, 443, 109
DOI
ScienceOn
|
7 |
Lee, K. H., et al. Wide field VI CCD photometry of globular cluster M92, 2002,, in preparation
|
8 |
Lee, C. W., Lee, H. M., Ann, H. B., & Kwon, K. H., 1999, Smoothed particle hydrodynamic simulations of Galactic gaseous disk with bar: Distribution and kinematic structure of molecular clouds toward the Galactic Center, ApJ, 513, 242
DOI
ScienceOn
|
9 |
Lee, H. M..1990, Tidal Densities of Globular Clusters and the Galactic Mass Distribution, JKAS, 23, 97
|
10 |
Lee, H. M., & Ostriker, J. P., 1986, The evolution and final disintegration of spherical stellar systems in a steady galactic tidal field, ApJ, 332, 123
|
11 |
Leon S., Meylan G., & Combes F. 2000, Tidal tails around 20 Galactic globular clusters. Observational evidence for gravitational disk/bulge shocking, A&A, 359, 907
|
12 |
MaKINO, J., 1991, A Modified Aarseth Code for GRAPE and Vector Processors, PASJ, 43, 859
|
13 |
Oh K. S., & Lin, D. N. C. 1992, Tidal evolution of globular clusters. II - The effects of Galactic tidal field and diffusion, ApJ, 386, 519
DOI
|
14 |
Spitzer, L. Jr. 1987, Dynamical Evolution of Globular Clusters (Princeton: Princeton University Press)
|
15 |
Caldwell, J. A. R., & Ostriker, J. P. 1981, The mass distribution within our Galaxy - A three component model, ApJ, 251, 61
DOI
|
16 |
Aarseth, S. J. 1999, From NBODYl to NB0DY6: The growth of an industry, PASP, 111, 1333
DOI
ScienceOn
|
17 |
Aarseth, S. J., Henon M., & Wielen R. 1974, A comparison of numerical methods for the study of star cluster dynamics, A&A, 37, 183
|
18 |
Ahmad A., & Cohen L. 1973, Random force in gravitational systems, APJ, 179, 885
DOI
|
19 |
Gnedin, O. Y., Lee, H. M., & Osthker, J. P. 1999, Effects of tidal shocks on the evolution of globular clusters, ApJ, 522, 935
DOI
ScienceOn
|
20 |
H$`{e}$non, M., 1961, Sur I'evolution dynamique des amas globulaires, Ann. d'Astrophys., 24, 369
|
21 |
Kim, E., Einsel, C., Lee, H. M., Spurzem, R., & Lee, M. G., 2002, Dynamical evolution of rotating stellar systems -II. Post-collapse, equal mass system, MNRAS, in press
|