We investigate dynamical evolution of globular clusters with multi-mass component under the Galactic tidal field. We compare the results with our previous work which considered the cases of single-mass component m the globular clusters. We find the followings: 1) The general evolutions are similar to the cases of single-mass component. 2) There is no evidence for dependence on the orbital phase of the cluster as in the case of single-mass component. 3) The escape rate in multi-mass models is larger than that in the single-mass models. 4) The mass-function depends on radius more sensitively in anisotropic models than in isotropic models.

A new cultivar ofDianthus caryophyIIus "Gamet" was selected from the progenies ofa cross "Master" and "97007-2"in 1998 at the National Horticultural Research Institute, Rural Development Administration. It was fmally selected in 2001 afterthe investigatio

A new cultivar ofDianthus caryophyUus "Pavo" was selected from the progenies ofa cross "Sarangbyul" and "TargetWhite" in 1997 at the National Horticultural Research Institute, Rural Development Administration. It was finally selected m 2001after the inves