We present BV CCD photometry for the open clusters Czernik 24 and Czernik 27. These clusters have never been studied before, and we provide, for the first time, the cluster parameters; reddening, distance, metallicity and age. Czernik 24 is an old open cluster with age 1.8 ± 0.2 Gyr, metallicity [Fe/H]=-0.41 ± 0.15 dex, distance modulus (m-M)0=13.1 ± 0.3 mag (d=4.1 ± 0.5 kpc), and reddening E(B-V)=0.54 ± 0.12 mag. The parameters for Czernik 27 are estimated to be age=0.63 ± 0.07 Gyr, [Fe/H]=-0.02 ± 0.10 dex, (m-M)0=13.8 ± 0.2 mag (d=5.8 ± 0.5 kpc), and E(B-V)=0.15 ± 0.05 mag. The metallicity and distance values for Czernik 24 are consistent with the relation between the metallicity and the Galactocentric distance of other old open clusters. We find the metallicity gradient of 51 old open clusters including Czernik 24 to be Δ[Fe/H]/ΔRgc = -0.064±0.009 dex kpc-1.

UBVIJHK photometry of the open cluster NGC 2194 are presented. Color-Magnitude diagrams of this cluster show well-defined main sequence and red giant clump. The main sequence also contains clear evidence of binary populations. Based on color-color diagrams, absolute magnitude of red giant clump, ZAMS fitting, and comparisons of observed color-magnitude diagrams with theoretical models, we derive following parameters for the cluster; reddening E(B-V)=0.44±0.04, age of log t ~8.8, and finally distance of (m-M)0=12.20±0.18.

Current instrumentation activities and the open user status of Okayama Astrophysical Observatory (OAO) are reviewed. There are two telescopes in operation and one telescope under reforming at OAO. The 188cm telescope is provided for open use for more than 200 nights in a year. The typical over-subscription rate of observation proposals for the 188cm telescope is ~ 1.5 - 2. The 50cm telescope is dedicated to ɤ-ray burst optical follow-up observation and is operated in collaboration with Tokyo Institute of Technology. The 91cm telescope will become a new very wide field near-infrared camera in two years. The high-dispersion echelle spectrograph (HIDES) is the current primary instrument for the open use of the 188cm telescope. Two new instruments, an infrared multi-purpose camera (ISLE) and an optical low-dispersion spectrograph (KOOLS), are now under development. They will be open as common use instruments in 2006.

동해의 심층수 형성은 크게 대륙주변부 대류와 외양대류에 의한 것으로 알려져 있다. Vladivostok 연안과 subpolar front사이에서 겨울철에 발생하는 심층수의 형성은 외양대류에 의한 가능성이 높은 것으로 설명되고 있으며, 침니 현상이 이러한 결과를 됫받침 하고 있다. 본 논문에서는 외양대류에 의한 심층수 형성과정의 초기단계 즉 침니 현상의 전 단계에 나타나는 현상을 포텐셜 와도, 지형류, 수온, 염분, 용존산소의 분포로부터 확인하였다. 포텐셜와도의 분포에서 나타난 와동류는 Vladivostok 연안과 subpolar front 사이에 위치하며, 와동류의 분포 위치는 겨울철 심층수 형성 가능성이 높은 해역과 잘 일치한다. 특히 대륙의 지형적인 특성으로 인한 바람장의 변화는 본 연구에서 나타난 시계반대방향의 와동류가 형성될 수 있음을 보여주며, 그 결과로 나타나는 dome 구조의 밀도 분포는 외양대류의 초기 단계에서 나타나는 현상을 잘 보여준다.

Open-rectangular plan Hanok is one of the major types that compose the urban tissues of Bukchon, a typical traditional residential area in Seoul. Through the comparison of the cadastral map of 1912 and the aerial photograph of 1962, the paper has given the outline of the and the distribution of Open-rectangular plan Hanok at Bukchon. And the paper defines the characteristics of Open-rectangular plan Hanok at Bukchon as followings. First, Open-rectangular plan Hanok at Bukchon is the mutated type of Open-rectangular plan Hanok in Kyong-gi Province. Second, the composition and characteristics of Bakat-chae and outer-courtyard have been changed through the adaptation itself to the compact lots of urban neighborhood. Third, the composition and characteristics of An-chae has not been changed except the inner corner bay, that gives the lights and view to An-bang through the window. And the comparison and observation of four examples, the paper defines the identities of Open-rectangular plan Hanok at Bukchon. The partial transformation comes from the conflicts and adjustments with the structure of alley and the topographical condition of lots.

A new method has been developed to solve the star cluster membership problem. It is based on synthetic photometry employing the Black Body concept as stellar radiation simulator. Synthetic color-magnitude diagram is constructed showing the main sequence band and the positions of binary star systems of combinations of various components through different photometric tracks. The method has been applied to the Hyades. The cluster membership problem has been re-appraised for the cluster (both single and binary) stars. For the binary members, the components' spectral types have been derived by the method. The results obtained agree very well with those found in literature, The method is simpler than the others and can be developed to undertake other cases as multiple star systems.

본 연구는 도축돈의 난소로부터 난자를 채취하여 체외배양시킨 후 세포 안정제와 원심분리 그리고 OPS를 이용한 유리화동결 하였다. 동결 융해한 수정란을 경산돈에 외과적 또는 비외과적으로 이식하여 자돈을 생산하는 것을 목적으로 수행하였다. 도축돈 난소로부터 채란되어진 돼지 미성숙난은 Funahashi 등(1994) 방법에 따라 체외 성숙-수정-배양하였다. 체외배양액은 glucose-free NCSU 23을 이용하였으며, 5일째에 10% Fatal bovin