• 천문학회보
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• 제45권1호
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• pp.33.2-33.2
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• 2020

Our HI monster sample is a set of local HI-rich galaxies identified by the ALFALFA survey (Arecibo Legacy Fast Survey ALFA) at z<0.08. Intriguingly, they are also found with a relatively large molecular gas reservoir compared to the galaxies with similar stellar mass and color, yet their star formation rate is quite comparable to normal spirals. This makes our HI monsters good candidates of galaxies in the process of gas accretion which may lead to the stellar mass growth. One feasible explanation for their relatively low star formation activity for a given high cool gas fraction is the gas in monsters being too turbulent to form stars as normal spirals. In order to verify this hypothesis, we probe the molecular gas kinematics of 10 HI monsters which we observed using the Atacama Large Millimeter/sub-millimeter Array (ALMA). We utilize the tilted ring model to investigate what fraction of the molecular gas in the sample is regularly and smoothly rotating. In addition, we model the molecular gas disk using the GALMOD package of the Groningen Image Processing System (GIPSY) and compare with the observations to identify the gas which is offset from the 'co-planar differential rotation'. Based on the results, we discuss the possibility of gas accretion in the sample, and the potential origin of non-regularly rotating gas and the inefficient star formation.

• 천문학회보
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• 제36권1호
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• pp.62.1-62.1
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• 2011

Warp phenomenon seems to be ubiquitous among spiral galaxies, and a a number of mechanisms have been suggested as the origin including cosmic infall and tidal interactions. In this work, we compare warp characteristics of cluster spirals and the ones in the field in order to investigate the influence of environment on warping, in particular of gas disks. We make use of a tilted-ring modeling (TRM) method to VLA HI (21cm) data cubes of carefully selected 20 spiral galaxies in the Virgo cluster. The TRM allows us to probe kinematics, e.g., inclination, position angle, and velocity dispersion of HI disks. We compare the properties of each tilted-ring component to mean properties based on optical images. In this contribution, we present preliminary yet important findings on the warp characteristics of spiral galaxies in dense environment, and discuss possible origins of those kinematical structures.

• 한국지구과학회지
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• 제28권7호
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• pp.847-856
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• 2007

행성상성운 NGC 6881은 4극자형태를 이루고 있고 JET이 영상에 나타난다. Lick 천문대에 있는 Hamilton Echelle Spectrograph(HES)을 사용하여 관측한 가시광 영역의 방출선 스펙트럼의 선윤곽을 연구하였다. 우리가 연구하는 HES 분광 자료는 직경이 4초각인 영역의 안쪽에서 관측된 것이다. IRAF와 StarLink/Dipso분석프로그램을 사용하여 HI, HeI, HeII, [OIII], [NII], [ArIII], [SII], [SIII] 등의 강한 선들의 선윤곽을 통해 팽창속도를 얻었다. HI선의 경우 단일 정상을 보이는 반면, He과 다른 금지선들은 두 개의 정상 분포가 겹치는 특성을 보였다. 가스 유출 속도는 중심별의 복사압에 의해 바깥쪽으로 갈수록 가속되는 것으로 분석되었다. 우리는 팽창속도자료를 통해, HST 영상에서 보여진 중심부분의 세 개의 고리는 양극콘(HI 선등에 나타남)과 고리(He, [SIII]선에 특성이 보임)의 복합 구조가 투영된 것으로 결론지었다.

• 대한치과보철학회지
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• 제20권1호
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• pp.75-81
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• 1982

The purpose of this study was to compare the marginal fitness between Ni-Cr alloy and type III gold alloy, according to two finishing line, chamfer and shoulder. As experimental materials, author selected type III gold alloy and Ni-Cr alloy (Hicrown) which were popularly used in Korea for the full cast crown. Author prepared the wax patterns with milled stainless steel die and ring. The wax patterns were invested, burnouted, and casted. The maginal discrepancy was measured with scanning electron microscope. Author obtained the following results from this study. 1. The maginal fitness of Type III gold alloy was not significantly different from that of Ni-Cr alloy (Hi-crown). 2. There is no significant difference between chamfer and shoulder in case of Type III gold alloy. 3. The maginal fitness of chamfer type is significantly superior to that of shoulder type in the Ni-Cr alloy (Hi-Crown).

• 대한전자공학회논문지SD
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• 제46권12호
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• pp.105-112
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• 2009

본 논문에서는 $0.35{\mu}m$ Bipolar-CMOS-DMOS(BCD)공정으로 설계한 스마트 파워 IC 내의 가드링 코너 영역에서 발생하는 비정상적인 정전기 불량을 관측하고 이를 분석하였다. 칩내에서 래치업(Latch-up)방지를 위한 고전압 소자의 가드링에 연결되어 있는 Vcc단과 Vss 사이에 존재하는 기생 다이오드에서 발생한 과도한 전류 과밀 현상으로 정전기 내성 평가에서 Machine Model(MM)에서는 200V를 만족하지 못하는 불량이 발생하였다. Optical Beam Induced Resistance Charge(OBIRCH)와 Scanning Electronic Microscope(SEM)을 사용하여 불량이 발생한 지점을 확인하였고, 3D T-CAD 시뮬레이션으로 원인을 검증하였다. 시뮬레이션 결과를 통해 Local Oxidation(LOCOS)형태의 Isolation구조에서 과도한 정전기 전류가 흘렀을 때 코너영역의 형태에 따라 문제가 발생하는 것을 검증하였다. 이를 통해 정전기 내성이 개선된 가드링 코너 디자인 방법을 제안하였고 제품에 적용한 결과, MM 정전기 내성 평가에서 200V이상의 결과를 얻었다. 통계적으로 Test chip을 분석한 결과 기존의 결과 대비 20%이상 정전기 내성이 향상된 것을 확인 할 수 있었다. 이 결과를 바탕으로 BCD공정을 사용하는 칩 설계 시, 가드링 구조의 정전기 취약 지점을 Design Rule Check(DRC) 툴을 사용하여 자동으로 찾을 수 있는 설계 방법도 제안하였다. 본 연구에서 제안된 자동 검증방법을 사용하여, 동종 제품에 적용한 결과 24개의 에러를 검출하였으며, 수정 완료 제품은 동일한 정전기 불량은 발생하지 않았고 일반적인 정전기 내성 요구수준인 HBM 2000V / MM 200V를 만족하는 결과를 얻었다.

• 대한수학회지
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• 제41권3호
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• pp.501-511
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• 2004

We prove the Hyers-Ulam-Rassias stability of the Davison functional equation f($\chi$y) + f($\chi$ + y) = f($\chi$y + $\chi$) + f(y) for a class of functions from a ring into a Banach space and we also investigate the Davison equation of Pexider type.

• 천문학회보
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• 제41권2호
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• pp.62.2-62.2
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• 2016

We present a newly developed algorithm based on a Bayesian method for 2D tilted-ring analysis of disk galaxies which operates on velocity fields. Compared to the conventional ones based on a chi-squared minimisation procedure, this new Bayesian-based algorithm less suffers from local minima of the model parameters even with high multi-modality of their posterior distributions. Moreover, the Bayesian analysis implemented via Markov Chain Monte Carlo (MCMC) sampling only requires broad ranges of posterior distributions of the parameters, which makes the fitting procedure fully automated. This feature is essential for performing kinematic analysis of an unprecedented number of resolved galaxies from the upcoming Square Kilometre Array (SKA) pathfinders' galaxy surveys. A standalone code, the so-called '2D Bayesian Automated Tilted-ring fitter' (2DBAT) that implements the Bayesian fits of 2D tilted-ring models is developed for deriving rotation curves of galaxies that are at least marginally resolved (> 3 beams across the semi-major axis) and moderately inclined (20 < i < 70 degree). The main layout of 2DBAT and its performance test are discussed using sample galaxies from Australia Telescope Compact Array (ATCA) observations as well as artificial data cubes built based on representative rotation curves of intermediate-mass and massive spiral galaxies.

• 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.

• 한국지형학회지
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• 제18권3호
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• pp.1-10
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• 2011

지오사이트로서의 산방산과 용머리 해안은 그 범위가 상당히 넓고 다양한 코스를 통해 관광객들이 접근하고 있다. 따라서 이를 고려하여 이 곳의 지오사이트 안내표지판은 현재보다 최소 2배 이상 늘리고 설치 장소를 포인트별로 분산시킬 필요가 있다. 안내표지판의 제목은 '산방산 용암원정구', '용머리 응회환', '산방산 용암원정구와 용머리 응회환의 관계' 등 세가지로 나누는 것이 바람직하다. 안내표지판은 관광객들이 짧은 시간에 한눈에 읽어내야 하므로, 그 내용은 서술이 체계적이고 간단, 명료해야한다. 연구 지역의 뷰포인트는 크게 산방산 조망, 용머리해안 조망, 산방산과 용머리해안 동시 조망 등 3가지로 나눌 수 있다. 이들 각 조망별 뷰포인트는 각각 3곳씩 모두 9곳에 설정이 가능하다. 산방산과 용머리 해안 지오사이트 내에서는 산방산과 용머리 응회환의 층서 경계부, 포획 현무암, 마린 포트홀, 타포니, 엇갈린 경사퇴적층 등 5곳의 소주제 경관이 관찰된다. 이들 소주제들은 해당 지오사이트는 물론 전체 지오파크를 유기적으로 이해하는데 큰 도움이 되므로 적극적으로 발굴하여 활용할 필요가 있다.

• Bulletin of the Korean Chemical Society
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• 제29권10호
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• pp.1946-1950
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• 2008

The synthesis of new 5-cyano-1,1-disubstituted phthalans having aromatic and aminoalkyl groups at C-1 position of phthalan ring and their biological evaluation are described. Most compounds exhibited comparable ejaculation-retarding effects to citalopram. Of these compounds, 3a, e showed excellent efficacy in delaying ejaculation.