• 천문학회보
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• 제45권1호
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• pp.51.1-51.1
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• 2020

The Rosette Nebula is the most actively star-forming region in the Monoceros OB2 association. This region hosts more than three stellar groups, including the most populous group NGC 2244 at the center of the region and the smaller stellar groups around the border of the H II bubble. To trace their formation process, we investigate the kinematic properties of these groups using the Gaia astrometric data and high-resolution spectra taken from observation with Hectochelle on MMT. The proper motions of stars in NGC 2244 show a pattern of radial expansion. The signature of cluster rotation is also detected from their radial velocities. On the other hand, the small groups appear to be physically associated with some clouds at the ridge of the H II region. Among them, the group near the eastern pillar-like gas structure shows the signature of feedback-driven star formation. In this presentation, we will further discuss the formation process and dynamical evolution of the stellar groups in the Rosette Nebula, based on the observation and results of N-body simulations.

• 천문학논총
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• 제22권4호
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• pp.97-101
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• 2007

We are often faced with the task of having to estimate the hydrogen and helium ionizing luminosities of massive stars in the study of H II regions and the warm ionized medium (WIM). Using the results of the most complete compilation of stellar parameters (the effective temperature, stellar radius and surface gravity) and the latest Kurucz stellar atmosphere models, we calculate the ionizing photon luminosities in the $H^0\;and\;He^0$ continua from O3 to B5 stars. We compared the theoretical Lyman-continuum luminosity with the observationally inferred luminosity of the H II region around ${\alpha}$ Vir, and found that the theoretical value is higher than the observed value in contrast to the eariler result.

• 대한의용생체공학회:학술대회논문집
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• 대한의용생체공학회 1996년도 춘계학술대회
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• pp.203-206
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• 1996

To understand the local fluid dynamics for different desists of Fontan operation, five models were made out of Pyrex glass to facilitate in-vitro study. Model I, II and III have same position of the center of the anastomosis of the IVC( inferior vena cava) with that of the SVC(superior vena cava), but Model IV and V have 10 mm offset between them. Also the anastomotic junction angles are different(Model I and $IV:90^{\circ}$, Model II and $V:70^{\circ}$, Model $III:45^{\circ}$). These models were then connected to a flow loop for flow visualization study. In Model I any dominant vortex was not seen in the central region of the juntion, but a large unstable vortex was created in the Model II and III. In Model IV and V a significant stagnation region was created in the middle of the offset region. It also showed that the flow direction from the IVC and SVC to the LPA(left pulmonary artery) and RPA(right pulmonary artery) highly depends on the offset of the junction rather than the anastomotic junction angle.

• 생명과학회지
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• 제14권6호
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• pp.1009-1017
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• 2004

인간유래 시알산전이효소 유전자들의 특이적 발현과 그들의 mRNA isoform의 생성에 대한 조절기구를 이해하기 위하여 5종류의 human 시알산전이효소 유전자(hST3Cal II, hST8Sia II, hST8Sia III, hSTS8Sia IV, hST8Sia V)들의 게놈구조를 분석하였다. hST3Gal II 유전자는 17 kb이상의 게놈상에 46 bp에서 1017 bp의 길이를 가진 exon이 6개로 이루어져 있고, hST8Sia III유전자는 10 kb이상의 게놈상에 125bp에서 2023bp의 길이를 가진 exon이 4개로 이루어져 있어 다른 human 시알산전이효소 유전자들보다 짧고 단순한 구조를 가지고 있었다. 반면에 다른 3종류의 유전자(hST8Sia II, hST8Sia IV, hST8Sia V)들은 70 kb이상의 게놈상에 5개이상의 exon으로 이루어져 있으며, 5종류 모두 exon-intron boundary는 GT-AG rule을 나타내고 있었다. 특히 모든 시알산전이효소에 고도로 보존되어 있는 sialylmotif L은 hST8Sia III유전자에서는 하나의 exon에 존재하는 반면에, 다른 시알산전이효소 유전자에서는 분리된 exon에 존재하여 exon의 구조적 다양성을 나타내고 있다. 또한, 본 연구에서는 5'-RACE와 cap site hunting법에 의해 hST3Gal II 유전자의 전사개시점을 결정하였다.

• 동력기계공학회지
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• 제4권1호
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• pp.81-87
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• 2000

In this study, CT specimens were prepared from ASTM SA516 Gr. 70 which was used for pressure vessel plates for room and low temperature service. And we got the following characteristics from fatigue crack growth test carried out in the environment of room and low temperature at $25^{\circ}C,\;-60^{\circ}C,\;-80^{\circ}C\;and\;-100^{\circ}C$ and in the range of stress ratio of 0.05 by means of opening mode displacement. At the constant stress ratio, the threshold stress intensity factor range ${\Delta}K_{th}$ in the early stage of fatigue crack growth (Region I) and stress intensity factor range ${\Delta}K$ in the stable of fatigue crack growth (Region II) was increased in proportion to descend temperature. It assumed that the fatigue resistance characteristics and fracture strength at low temperature is considerable higher than that of room temperature in the early stage and stable of fatigue crack growth region. The straight line slope relation of logarithm $d{\alpha}/dN\;-{\Delta}K$ in Region II, that is, the fatigue crack growth exponent m increased with descending temperature at the constant stress ratio. It assumed that the fatigue crack growth rate $d{\alpha}/dN$ is rapid in proportion to descend temperature in Region II and the cryogenic-brittleness greatly affect a material with decreasing temperature.

• 천문학회지
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• 제36권2호
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• pp.55-60
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• 2003

In Lee, Kang & Byun (2001) the discovery of Raman scattered 6545 A feature was reported in symbiotic stars and the planetary nebula M2-9. The broad emission feature around 6545 A is formed as a result of Raman scattering of He II n = 6 $\to$ n = 2 photons by atomic hydrogen. In this paper, we introduce a method to compute the equivalent width of He II $\lambda$ 1025 line and present an optical spectrum of the symbiotic star RR Telescopii as an example for a detailed illustration. In this spectrum, we pay attention to the broad H$\alpha$ wings and the Raman scattered He II 6545 feature. The broad Ha wings are also proposed to be formed through Raman scattering of continuum around Ly$\beta$ by Lee (2000), and therefore we propose that the equivalent width of the He II $\lambda$ 1025 emission line is obtained by a simple comparison of the strengths of the 6545 feature and the broad H$\alpha$ wings. We prepare a template H$\alpha$ wing profile from continuum radiation around Ly$\beta$ with the neutral scattering region that is supposed to be responsible for the formation of Raman scattered He II 6545 feature. Isolation of the 6545 feature that is blended with [N II] $\lambda$ 6548 is made by using the fact that [N II] $\lambda$ 6584 is always 3 times stronger than [N II] $\lambda$ 6548. We also fit the 6545 feature by a Gaussian which has a width 6.4 times that of the He II $\lambda$ 6527 line. A direct comparison of these two features for RR Tel yields the equivalent width $EW_{Hel025} = 2.3{\AA}$ of He II $\lambda$ 1025 line. Even though this far UV emission line is not directly observable due to heavy interstellar extinction, nearby He II lines such as He II $\lambda$ 1085 line may be observed using far UV space instruments, which will verify this calculation and hence the origins of various features occurring in spectra around H$\alpha$.

• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2006년도 한국우주과학회보 제15권2호
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• pp.177-180
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• 2006

우리은하 중심부의 Sgr A East에 인접한 별탄생 지역인 수소이온화영역 A주변에서 충격파가 별탄생에 미치는 영향을 조사하기 위하여 $2.1218{\mu}m$ 수소분자 방출선($H_2$ 1-0 S(1))을 관측하였다. 관측은 3.8m United Kingdom Infrared Telescope(UKIRT)에서 에셀 분광 모드의 Cooled Grating Spectrometer 4(CGS4)를 사용하여 각분해능 약 2arcsec, 파장 분해능 약 18km s^{-1}$으로 수행 되었다. 검출된 수소분자선을 공간적인 구조와 속도 분포의 측면에서 각각 전파 연속선 방출광 및 암모니아 방출광과 비교한 결과, 수소분자 방출광은 Sgr A East의 충격파와 무관하며 수소이온화영역 자체의 분자해리영역에서 방출된 것이라는 결론에 도달하였다. 이는 해당 지역에서의 별탄생이 Sgr A East의 충격파에 의해 촉발된 것이 아니라는 것을 의미한다.

• Bulletin of the Korean Chemical Society
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• 제6권4호
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• pp.214-217
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• 1985

Platinum(II) complexes of R-2,2'-diaminobinaphthyl (R-dabn), [Pt(R-dabn)(H2O)2]Cl2, [Pt(R-dabn)(R-Pn)]Cl2, [Pt(R-dabn)(R-bn)]Cl2, and platinum(II) complexes of S-2,2'-diaminobinaphthyl (S-dabn), [Pt(S-dabn)(H2O)2]Cl2, [Pt(S-dabn)(S-Pn)]Cl2, and [(Pt(S-dabn)(S-bn)]Cl2 have been prepared. (R-Pn and S-Pn are, respectively R- and S isomer of 2,3-diaminobutane). R-Pn and S-bn are, respectively R and S isomer of 2,3-diaminopropane). In the vicinity of the B-absorption band region of dabn, the circular dichroism spectra of platinum(Ⅱ) complexes of R-dabn series show a positive B-band followed by a negative higher energy A-band, which is generally understood as the splitting pattern for a ${\lambda}$ conformation, while the circular dichroism spectra of platinum(Ⅱ) complexes of S-dabn series show a negative B-band followed by a positive higher energy A-band in the long-axis polarized absorption region as expected for a $\delta$ conformation.

• International Union of Geodesy and Geophysics Korean Journal of Geophysical Research
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• 제23권1호
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• pp.34-38
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• 1995

A diagnostic study on the summertime air mass thunderstorms occurring in the middle region of South Korea was made by analyzing the data of surface and upper air observations as well as the surface and upper level weather charts. The key parameters used in the present study are the amount of precipitable water below 850 hPa level, the vertical profiles of water vapor content and wind, and both the temperature difference and the equivalent potential temperature difference between 850 hPa and 700 hPa levels. It is found from this study that the summertime air mass thunderstorms in the middle region of South Korea can be classified into two distinct types, type I and type II. The thunderstorms of type I occur under the atmospheric conditions of high moisture content, low vertical wind shear in low levels, and conditional instability between 850 hPa and 700 hPa levels. On the other hand, the thunderstorms of type II occur under the atmospheric conditions of less moisture content, higher wind shear and conditional instability. Furthermore, our study suggests that atmospheric instability and the amount of water vapor below 850 hPa level are complementary in the development of air mass thunderstorms. The complementary nature between these two parameters may be an explanation for the thunderstorm development in the areas of low atmospheric water vapor content such as the plains of eastern Colorado.

• 융합신호처리학회논문지
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• 제13권2호
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• pp.83-90
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• 2012

본 논문에서는 NIOS II 임베디드 플랫폼을 기반으로 하는 지능형 영상 감시 시스템을 구현하였다. 지금까지의 입베디 드 기반의 영상 감시 시스템들은 하드웨어의 의존도가 높아 특정한 목적에 제한되는 단점이 있었다. 이러한 한계를 개 선하기 위하여, 필자들은 그 응용의 목적에 따라 폭 넓게 적용 가능한 유연성이 높은 임베디드 플랫폼을 구현하였다. 소프트웨어 중심 프로그래밍 기법의 주요 문제점인 고속 처리를 위하여, 핵심 부분인 하드웨어 플랫폼에서 SOPC형 NIOS II 임베디드 프로세서와 영상처리 알고리즘을 소프트웨어 프로그래밍과 C2H(The Altera NIOS II C-To-Hardware(C2H) Acceleration Compiler) 컴파일러를 사용하는 하드웨어 프로그래밍을 통합하여 시스템의 성능을 향상 시켰다. 그리고 NIOS II 임베디드 프로세서 플랫폼을 중심으로 각각의 디바이스 인터페이스를 통합 관리하는 서버 시스템을 구축하고, 사용자의 접근 효율을 높이기 위해 네트워크상에서 제어하는 기능을 추가하였다.본 시스템을 영상 감시를 위한 지정된 구역에 설치하여 시험하고 그 성능을 평가하였다.