• 천문학회보
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• 제43권2호
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• pp.60-60
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• 2018

It has been known that XZ CMi is a near-contact binary composed of a hotter and more massive main-sequence primary star close to its Roche-lobe and a Roche-lobe filling giant/subgiant secondary star. There still exist, however, many discordant matters among the previous investigators: diverse mass ratios and temperatures ranging from 0.38 to 0.83 and from 7,000 K to 8,876 K, respectively. In order to make a contribution to the two confusions we conducted spectroscopic and photometric observations. A total of 34 high-resolution spectra were obtained during 4 nights from 2010 and 2018 with the Bohyunsan Optical Echelle Spectrograph (BOES) at the Bohyunsan Optical Astronomy Observatory (BOAO). In parallel, BVRI multi-band photometric observations were carried out 5 nights in 2010 at Sobaeksan Optical Astronomy Observatory (SOAO). In this presentation, we present physical parameters of XZ CMi through the simultaneous analyses of new double-lined radial velocity curves and new light curves. We will also briefly discuss the evolutionary status of the system.

• 대한치과보철학회지
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• 제38권2호
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• pp.214-225
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• 2000

The purpose of this study was to investigate the effects of investing conditions on the marginal discrepancy of conical telescope outer crown with Co-Cr-Ti alloy(Dentitan) and to compare the marginal discrepancy and the retention force of outer crowns using different pattern materials(plastic foil, casting wax, pattern resin). To evaluate the effects of investing conditions on the marginal discrepancy, patterns with plastic foil were invested under three different liquid/powder ratio conditions using phosphate bonded investment(Univest-nonprecious): standard, 10% decreased and 10% increased. At each liquid/powder ratio condition, metal ring was lined with single or double layers of ceramic ring liner. The marginal discrepancy of outer crown at different investing conditions was measured by ${\times}100$ compact measuring microscope(STM5, Olympus, Japan). For measurement of the marginal discrepancy and the retention force of outer crown using different pattern materials, the investing condition of 10% decreased liquid/powder ratio and double layers of ring liner was selected because this investing condition resulted in the best fit of outer crown. Marginal discrepancy was measured in the same way above and retention force on universal testing machine. Under the conditions of this study, the following conclusions were drawn: 1. The thickness of ring liner had more influence on the marginal discrepancy of outer crown than the liquid/powder ratio, and the acceptable marginal fitness could not be expected at the investing condition directed by investment manufacturer 2. There were no differences in the marginal discrepancy of outer crown among three different pattern materials(P>0.05). 3. Casting wax showed the greatest retention force(1640g) of outer crown, followed by pattern resin(1110g), plastic foil(820g). However, there was no significant difference between plastic foil and pattern resin(P>0.05). 4. Plastic foil showed the least variation in marginal discrepancy and retention force.

• Pediatric Gastroenterology, Hepatology & Nutrition
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• 제13권1호
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• pp.75-80
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• 2010

장중첩증이 재발한 15개월 여아에서 초음파 검사에서 병적 선두로 생각되는 낭성 종괴를 확인하였고 이중벽 징후와 인접한 소장 사이에 Y자 형상의 저반향 경계를 가지고 있어 중복 낭종으로 의심하였다. 이후 절제술을 시행하여 조직병리검사에서 인접한 회장과 근육층을 공유하고 낭종의 바깥쪽으로는 인접한 장 점막상피 조직과 안쪽으로는 이소성 위 점막 조직이 관찰되는 중복 낭종으로 확진되어 문헌 고찰과 함께 보고하는 바이다.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 1992년도 한국우주과학회보 제1권1호
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• pp.15-15
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• 1992

AQ Cassiopeiae (BD+61`0242, uv=10, Sp=B3+Bg) is a totally eclipsing binary system with the obital period of about 12 days. 71 was observed for 15 nights in 1985 with the1.8-m telescope at the DAO, employing a Reticon and a three-stage image tube attached to the spectrograph. And also, photometric observations of AQ Cas had been made inUBv for six years from 1982 to 1988 at Yonsei University Observatory(YUO). This work includes UBV observations obtained at YUO as a part of The Ten-Year Observing Program(1982-1992). Double lined radial, velocity curves and Ufv light curves of AQC as are constructed. The light curves and radial velocity curves show a strong evidence of circumstellar matter or mass stream. It is clear at the phases of just outside externaleclipse contacts, particularly at phase 0.8-0.9, shown in Figures 1 and 2. A solution by combining the radial velocity and photometric curves of the binary was obtained with the Wilson-Devinney Code. We found that the system is semi-detached with the coolcomponent filling its Roche lobe. The absolute dimensions of AQ Cas are calculated. The result shows that this system consists of two massive and subgiant stars.

• Applied Microscopy
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• 제50권
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• pp.6.1-6.6
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• 2020

The cerebellum is a region of the brain that plays an important role in motor control. It is classified phylogenetically into archicerebellum, paleocerebellum and neocerebellum. The Purkinje cells are lined in a row called Purkinje cell layer and it has a unique dendritic branches with many spines. The previous study reported that there is a difference of synapse density according to the lobules based on large two-dimensional data. However, recent study with high voltage electron microscopy showed there was no differences in dendritic spine density of the Purkinje cell according to its phylogenetic lobule. We analyzed Purkinje cell density in the II, VI and X lobules by stereological modules and synaptic density was estimated by double disector based on Purkinje cell density in the molecular layer of each lobule. The results showed that there was significant difference in the Purkinje cell density and synapse number according to their phylogenetic lobules. The number of Purkinje cell in a given volume was larger in the archicerebellum, but synapse density was higher in the neocerebellum. These data suggest that cellular and synaptic organization of the Purkinje cell is different according to their phylogenetic background.

• Applied Microscopy
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• 제23권1호
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• pp.56-76
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• 1993

To investigate the histogenesis of tracheal epithelium in Sprague-Dawley strain rat, the author has used the fetal rats at the 16th, 18th, 20th and 22nd prenatal day and neonatal rats at the 1st and 7th day as well as rats at age of 5, 10 and 15 weeks after birth as experimental animals. Specimens were double stained with uranyl acetate and lead citrate for electron microscopic study. The results obtained were as follows; 1. At the 16th day of gestational age, ciliated cells were found in tracheal epithelium and light and dark ciliated cells possessing numerous mitochondria and smooth endoplasmic reticulum in the cytoplasm at the 22nd day of gestational age of the rat are observed. 2. At the 16th day of gestataional age, basal cells lying upon the basement membrane and having large numbers of glycogen particles in the cytoplasm, were found and at the 22nd day of gestational age, basal cells possessing numerous polysomes in the cytoplasm were observed. 3. At the 20th gestational age of the rat, microvillous cells possessing many rough endoplasmic reticulum and mitochondria as well as microvilli protruding into the lumen were found in tracheal epithelium. 4. At the 5th week after birth brush cell having profound filamentous strands and many pinocytic vesicles in the cytoplasm, was visible in the tracheal epithelium. 5. At the 15th week after birth large proportions of tracheal epithelium were lined with ciliated cells. Cosequently it is suggested that pseudostratified ciliated columnar epithelium was differentiated at the 16th day of gestational age, in addition cytoplasmic organelles of the microvillous and basal cells were matured at the 20th and 22nd gestational age, respectively and most of the part of the tracheal epithelium was lined with ciliated cells at the 15th week after birth.

• Journal of Astronomy and Space Sciences
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• 제24권2호
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• pp.99-110
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• 2007

W UMa형 접촉쌍성 CC Com을 소백산 천문대에서 61cm 망원경과 2K CCD 카메라로 2002년 3월 3일부터 4월 3일까지 3일간 측광관측하여 총 824개의 관측점(${\Delta}B$: 206점, ${\Delta}V$: 206점, ${\Delta}R$: 206점, ${\Delta}I$: 206점)을 얻었다. 우리의 관측점으로부터 9개의 새로운 극심시각(주극심: 6개, 부극심: 3개)을 산출하였다. 2004년 Wilson-Devinney(WD) 쌍성 모형 계산 프로그램으로 우리가 얻은 새로운 BVRI 광도곡선과 발표된 이중시선속도 곡선들을 결합하여 분석함으로서 CC Com의 제 물리요소를 새롭게 산출하였다. 광도곡선에 나타난 작은 비대칭을 반성에 고온 반점 2개를 도입하여 설명하였다.

• Journal of Astronomy and Space Sciences
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• 제23권3호
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• pp.177-188
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• 2006

소백산 천문대의 61cm 망원경과 2K CCD 카메라로 2003년 1월 6일부터 24일까지 5일간 WUMa형 접촉쌍성 V523 Cas를 측광판측하여 총 920개의 관측점(${\Delta}B$: 230점, ${\Delta}V$. 230점, ${\Delta}R$: 230점, ${\Delta}I$: 230점)을 얻었다. 우리의 관측점으로부터 9개의 새로운 극심시각(주극심: 5개, 부극심: 4개)을 산출하였다. 2004년도 Wilson-Devinney(WD) 쌍성 모형으로 우리가 얻은 새로운 BVRI 광도곡선과 Rucinski et al.(2003)의 시선속도 곡선을 결합하여 분석함으로서 V523 Cas의 제 물리요소를 새롭게 산출하였다. 광도곡선에 나타난 작은 비대칭을 온도가 높은 주성의 광구 표면에 차거운 흑점과 반성에 뜨거운 흑점을 가정하여 설명하였다.

• 대한수의학회지
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• 제48권3호
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• pp.311-316
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• 2008

A 7-year-old female Shih Tzu dog with lots of masses in the whole mammary gland was presented to the surgery department of the Veterinary Teaching Hospital in the Cheju National University. After surgical excision, all mammary samples were referred to Pathology Department of Veterinary Medicine. Grossly, masses were measuring up to $6.5{\times}4{\times}1cm$ and on cut surface of masses in right 1st, 3rd, 4th, 5th and left 1st, 3rd, 4th, 5th mammary masses were well delineated and firm, sulphur yellow, solid round to oval shape. Microscopically, most neoplastic sweat glands were severely proliferated in dermis and subcutis. Most tubules were lined by round to oval shaped epithelium with eosinophilic cytoplasm, hyperchromatic nuclei with high mitotic figures and severe central necrosis. The neoplastic epithelium also had PAS-positive diastase-resistant cytoplasmic granules, but negative with Perls iron stain. The left 2nd mass was well delineated, and had several dark brown areas and yellowish white glittered areas. Mass was well circumscribed with dense connective tissue. Neoplastic areas contained irregular sized mammary gland with papillary grown luminal epithelial cells in single or double cells layer with mitotic figures and small amounts of proliferated myoepithelial cells. Proliferated myoepithelial cells also produced slightly basophilic mucinous materials. Based on the gross, histopathologic and special staining characteristics, this dog was diagnosed as 90% of apocrine sweat gland aenocarcinoma and 10% mammary. complex adenomas in mammary masses. In our best knowledge, this is the first report for concurrent occurrence of apocrine sweat gland adenocarcinoma and mammary gland complex adenoma in mammary masses of the same dog.

• 대한지리학회지
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• 제39권4호
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• pp.633-642
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• 2004

본 연구의 목적은 규칙기반 모델링을 구성하여 하계망을 일반화하고자 하였다. 그 동안 지도 일반화에 대한 연구는 제한된 지도요소를 대상으로 선형사상의 형태변형을 위한 알고리즘 개발과 평가에 집중되었다. 규칙 기반 모델링은 지도제작 원리와 공간현상의 분포패턴을 분석하여, 그 결과를 일반화 과정에 적용하기 때문에 기존의 일반화 알고리즘 개선에 도움이 된다. 규칙기반 모델링은 다양한 지도요소들을 대상으로 일반화를 적용할 수 있고, 디지털 환경하에서 다축척 지도제작에 효과적이다. 본 연구에서 개발된 하계망 규칙기반 모델링은 일반화 규칙, 중심선 추출 그리고 선형사상 일반화 알고리즘으로 구성된다. 일반화를 적용하기 앞서, 하계망은 논리적 오류를 최소화하기 위해 저수지와의 연결관계를 분석하였다. 모델을 적용한 결과, 108개의 실폭 하천 중 17개 하천이 중심선으로 추출되었다. 하천의 총길이는 1:25,000에서 17%, 1:50,000에서는 29%로 감소하였다. 선형사상 일반화를 위해 개발된 Simoo 알고리즘은 Douglas-Peucker 알고리즘과 비교하였다. Doug]as-Peucker 알고리즘은 자료점 간격과 편각이 커지게 되어 선의 형태가 거칠어지는 반면, Simoo 알고리즘에서 선형사상은 축척이 감소함에 따라 보다 완만해진다.