• 천문학회지
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• 제36권3호
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• pp.81-87
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• 2003

It is suggested that a flying-by star in a hot accretion disk may cool the hot accretion disk by the Comptonization of the stellar emission. Such a stellar cooling can be observed in the radio frequency regime since synchrotron luminosity depends strongly on the electron temperature of the accretion flow. If a bright star orbiting around the supermassive black hole cools the hot disk, one should expect a quasi-periodic modulation in radio, or even possible an anti-correlation of luminosities in radio and X-rays. Recently, the unprecedentedly accurate infrared imaging of the Sagittarius A$\ast$ for about ten years enables us to resolve stars around it and thus determine orbital parameters of the currently closest star S2. We explore the possibility of using such kind of observation to distinguish two quite different physical models for the central engine of the Sagittarius A$\ast$, that is, a hot accretion disk model and a jet model. We have attempted to estimate the observables using the observed parameters of the star S2. The relative difference in the electron temperature is a few parts of a thousand at the epoch when the star S2 is near at the pericenter. The relative radio luminosity difference with and without the stellar cooling is also small of order $10^{-4}$, particularly even when the star S2 is near at the pericenter. On the basis of our findings we tentatively conclude that even the currently closest pass of the star S2 is insufficiently close enough to meaningfully constrain the nature of the Sagittarius A$\ast$ and distinguish two competing models. This implies that even though Bower et al. (2002)have found no periodic radio flux variations in their data set from 1981 to 1998, which is naturally expected from the presence of a hot disk, a hot disk model cannot be conclusively ruled out. This is simply because the energy bands they have studied are too high to observe the effect of the star S2 even if it indeed interacts with the hot disk. In other words, even if there is a hot accretion disk the star like S2 has imprints in the frequency range at v $\le$ 100 MHz.

• 한국육종학회지
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• 제43권6호
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• pp.559-563
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• 2011

농촌진흥청 원예특작과학원에서는 2008년에 진한 자주색의 수출용 중 대형품종을 육성할 목적으로 1995년에 진자주색계 중형종 C. Miake'Pieta'와 중형종 진분홍색계 'Allstar Mariane' 품종을 교배하여 진자주색계 '퍼플스타'(Cymbidium 'Purple Star') 신품종을 개발하였다. 1996년부터 2007년까지 종자기내파종, 온실양성, 선발 그리고 특성검정으로 균일성, 안정성, 화색, 화수, 엽형 등이 우수하여 2008년 12월 농작물 직무육성 심의회를 거쳐 'Purple Star'로 명명하였다. 'Purple Star' 품종은 진자주색계(RHS, GP 186A)이며, 1개 꽃대에 10.7개의 소화가 착생하며 화폭이 약 7.6 cm로 크다. 꽃모양은 꽃받침과 꽃잎이 안쪽으로 약간 오므라드는 둥근 모양이고 꽃대는 반직립성이며 식물체 크기는 중형이다. 꽃은 보통재배시 1월 초순경부터 개화하는 중생종이며 잎 형태는 꼬임이 적은 반직립성이고 꽃대의 길이는 78.4 cm로 강건하며 수출용 재배에 적합하다.

• 항공우주기술
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• 제4권1호
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• pp.66-76
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• 2005

이 연구는 통계학적인 방법을 이용하여 별 추적기의 가시도를 해석하였다. 별 추적기의 시선벡터에 대한 함수로서, 몇 가지 위성 자세 모드 상태에서 임의의 위성의 위치로부터 별 추적기가 태양과 지구에 의해 가려지는 확률, 태양 전지판에 의해 별 추적기가 가려지는 확률, 태양 전지판에 의한 태양 빛의 반사 확률을 계산하였다. 별 추적기의 이용도가 가장 높은 영역을 찾아 별 추적기의 시선벡터 방향을 결정하였는데, 두개의 최적화된 별추적기의 배치는 각각 고도각 -40도, 방위각 -35도와 고도각 -40도, 방위각 -150도로 나타났다.

• 한국중재학회지:중재연구
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• 제27권4호
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• pp.133-156
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• 2017

The purpose of this paper is to take a countermeasure of the investment treaty arbitration that Lone Star claimed to the Korean government. In particular, this study suggests procedural measures to be prepared by the Korean government after the arbitration award. The actual remedy in ICSID arbitration is the annulment procedure of arbitration award. Therefore, this study analyzed the measures that the Korean government can prepare based on the annulment grounds: the inadequacy of the constitution of the arbitral tribunal, the excessive power of the arbitrator, the corruption of the arbitrator, and the serious violation of the rules. First, the Korean government should decide whether to proceed with the annulment procedure after the arbitration award. Second, if they decide to do it, they should review the grounds of annulment. For example, it is possible to analyze whether the relationship between the arbitrator and Lone Star can be properly in the constitution of the arbitral tribunal, whether Lone Star is eligible to apply for ICSID arbitration, or whether arbitration tribunal ignores the crucial evidence that can affect the arbitration award. Independently, the Korean government needs to discuss the investment arbitration appeal system in a long-term perspective.

• 천문학회보
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• 제40권2호
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• pp.53.3-53.3
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• 2015

We analyzed both HCN J=1-0 and HNC J=1-0 line profiles to study the inflow motions in different evolutionary stages of massive star formation; infrared dark clouds (IRDCs), high-mass protostellar object (HMPOs), and ultra-compact HII regions (UCHIIs). The infall asymmetry in HCN spectra seems to be prevalent throughout all the three evolutionary phases, with IRDCs showing the largest excess in blue profile. In the case of HNC spectra, the prevalence of blue sources does not appear, excepting for IRDCs. We suggest that this line is not appropriate to trace infall motion in evolved stages of massive star formation because of an astrochemical effect. This result spotlights the importance of considering chemistry in dynamical study in star-forming regions. The fact that the IRDCs show the highest blue excess in both infall tracers indicates that the most active infall occurs in the early phase of star formation, i.e., the IRDC phase rather than in the later phases. However, the UCHIIs is likely still accreting matters. We also found that the absorption dips of the HNC spectra in all blue sources are red--shifted relative to their central velocities. These red-shifted absorption dips may indicate the observational signature of overall collapse although observations with better resolutions are needed to examine this feature more in detail.

• International Journal of Contents
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• 제14권3호
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• pp.46-52
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• 2018

The objective of this study was to determine the status of star chart game applications in the Google play store in Korea. The share of game genres in paid and free star charts of game applications was searched. Also, the average reviewer's rating, average number of reviews, and average age rating based on the genre of paid and free star charts of game applications, and the average price of paid applications based on genre were analyzed. Hypothesis tests for the differences in average reviewer's rating, average number of reviews, average age rating according to the genre of game applications were performed. Also, hypothesis tests for the differences in average reviewer's rating, average number of reviews, average age rating between the paid and free game applications along with the hypothesis test for the differences in price according to the genre of paid game applications were performed. Lastly, hypothesis tests for the correlation between the start chart ranking and number of reviews in association with the correlation between the start chart ranking and reviewer's rating were performed. Statistically significant differences in average reviewer's rating, average number of reviews, average age rating according to the genre of game applications, and between the paid and free game applications were verified. However, the correlation between the start chart ranking and number of reviews in association with the correlation between the start chart ranking and reviewer's rating were not statistically significant.

• Journal of Astronomy and Space Sciences
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• 제11권1호
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• pp.115-130
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• 1994

구성물질에 영향을 받는 제5힘이 존재할 경우 별의 특성과 구조를 중성자성을 대상으로 살펴보았다. 중성자만으로 이루어진 축퇴된 중성자성의 크기, 질량및 구조는 변형된 토마스-페르미 방정식의 해로서 계산할 수 있고, 제5힘이 없을 경우와 같이 새로운 중성자성의 크기, 질량 및 구조가 제5힘의 상수와 중력상수 $\alpha$에 영향을 받고 있음을 알았다. 극히 상대론적인 경우 새로운 중성자성의 특성 질량인 챤드라세카르 질량, $M_{ch}\simeq(1-\alpha)^{-3/2}{m_{pl}}^3/m^2$ 은 물리법칙의 상수만으로 결정되는 것을 확인할 수 있었다. 그러나 실험 결과의 한계안에서 새로운 중성자성의 크기와 질랴의 변화량은 각각 $\alpha$/2 와 3$\alpha$/2 정도였다.

• 대한조선학회논문집
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• 제51권4호
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• pp.321-327
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• 2014

A wide scope of numerical simulations was performed to predict model-ship resistances by using STAR-CCM+ and OpenFOAM. The numerical results were compared with experimental measurements in towing tank to analyze statistical reliability of the present simulations. Based on the normal distribution of resistance errors in 113 cases of container carriers, tankers and very large crude-oil carriers, the confidence intervals of numerical error were estimated as [-2.64%,+2.32%] and [-1.82%, +1.87%] with 95% confidence in STAR-CCM+ and OpenFOAM, respectively. The resistance errors of liquefied natural gas carriers with single- and twin-skeg were confident in the ranges of [-2.51%,+2.64%] and [-2.29%, +1.46%], respectively. The grid uncertainty of resistance coefficients for KCS was also quantitatively analyzed by using a grid verification procedure. The grid uncertainty of OpenFOAM (5.1%) was larger than 4.4% uncertainty of STAR-CCM+ although OpenFOAM provided statistically more confident results than those of STAR-CCM+. It means that a grid system verified under a specific condition does not automatically lead to statistical reliability in general cases.

• 한국추진공학회:학술대회논문집
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• 한국추진공학회 2009년도 춘계학술대회 논문집
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• pp.381-384
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• 2009

해성I에 사용되는 공기흡입식 엔진은 초기 발사추력을 제공하는 부스터가 분리된 후 목표물까지 비행할 수 있는 2차 추진기관이다. 유도탄이 비행을 하는 동안 이동방향 및 고도를 원하는 대로 제어하기 위해서는 체계종합에서의 엔진 성능 검증이 필수적이며, 이를 위해 비행시험 전 지상에서 유도탄체계의 엔진시동시험을 수행하여야 한다. 본 논문은 해성I에 사용되는 공기흡입식 엔진의 성능검증을 위한 지상 시험, 평가 방법을 제시한다.

• 항공우주기술
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• 제11권2호
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• pp.87-95
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• 2012

본 기술논문에서는 고기동 고정밀 위성의 별 추적기 초기 점검 원격측정 데이터가 분석되었다. 최근에 발사된 위성은 고기동 고정밀 위성이므로 고도의 요구조건을 만족하기 위해 광학계, 전자부, 배플이 분리된 형태로 광학계 부분의 온도를 20 degC 근처로 유지하면서 저주파 오차 성능을 향상 시킨 프랑스 SODERN사의 SED36을 사용하였다. 본 논문에서는 위성으로부터 내려 받은 원격측정 데이터의 처리를 통해 초기 점검 상태, 요구 조건 만족 여부, 이상 현상 및 주요 임무 기동에서의 별 추적기 잡음각 성능 분석 결과를 제시하였다.