• 천문학회지
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• 제48권5호
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• pp.267-275
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• 2015

Simultaneous time monitoring observations of H₂O and SiO maser lines were performed toward the D-type symbiotic binary system V407 Cyg with the Korean VLBI Network single dish radio telescope. These monitoring observations were carried out from March 2, 2010 (optical phase ϕ = 0.0), 8 days before the nova outburst on March 10, 2010 to June 5, 2014 (ϕ = 2.13). Eight days before the nova outburst, we detected the SiO v = 1, 2, J = 1–0 maser lines which exhibited values of 0.51 K (∼ 6.70 Jy) and 0.71 K (∼ 9.30 Jy), respectively, while after the outburst we could not detect them on April 2 (ϕ = 0.04), May 5 (ϕ = 0.09), May 8 (ϕ = 0.09), or on June 5, 2010 (ϕ = 0.13) within the upper limits of our KVN observations. After restarting our monitoring observations, we detected SiO v = 2, J = 1–0 masers starting on October 20, 2011 (ϕ = 0.83) and detected SiO v = 1, J = 1–0 masers starting on December 22, 2011 (ϕ = 0.92). These results provide clear evidence of the interaction between the shock from the nova outburst and the SiO maser regions of the Mira envelope. The peak emission of SiO v = 1, 2, J = 1–0 masers always occurred at blueshifted velocities with respect to the stellar velocity except for that of SiO v = 1 at one epoch. These phenomena may be related to the redistribution of SiO maser regions after the outburst. The peak velocity variations of SiO masers associated with stellar pulsation phases show an increasing blueshifted trend during our monitoring interval after the outburst.

• 천문학회보
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• 제42권1호
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• pp.54.1-54.1
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• 2017

The UKIRT Wide-field Infrared survey for Fe+(UWIFE) is an unbiased survey of the first Galactic quadrant, with narrow-band filter centered on $1.644{\mu}m$. This survey covers $7^{\circ}$ < l < $62^{\circ}$ and |b| < $1.5^{\circ}$, where active interaction of stars and interstellar medium is expected. With median seeing of 0.8 arcsec, 5 - sigma detection limit of 18.7 mag and surface brightness limit of $8.1{\times}10^{-20}W\;m^{-2}arcsec^{-2}$, this survey gives an opportunity to statistically study Galactic [Fe II] - emitting sources for the first time. In order to identify Ionized Fe Objects (IFOs) in survey area systematically, we conducted visual inspection and automatic detection simultaneously. Total of ~300 extended IFOs are identified, most of them are found out to be part of supernova remnants (SNRs), young stellar objects, HII regions and planetary nebulae. The majority of IFOs are new discoveries which reveal shocked structures in high-extinction region. Spatial distribution of IFOs suggest that they trace Galactic structure. As a part of spectroscopic follow-up, we observed SNR candidate IFO J183740.829-061452.41 with IGRINS (Immersion Grating Infrared Spectrograph, Yuk+2010), mounted on 2.7m Harlan Smith telescope. This unknown arc-like, 6'-long IFO is coincident with inner part of radio continuum loop G25.8+0.2, which has been known as HII region. However, interior of this radio shell is filled with diffuse soft X-ray emission, and possible association of hard X-ray pulsar / pulsar wind nebula makes the nature of the IFO unclear. The H and K-band 2D spectrum shows shock-ionized [Fe II] filaments, which is apart from photoionized HII filaments. In this presentation we present basic statistics of newly identified IFOs, as well as the follow-up study of IFO J183740.829-061452.41.

• 한국전산유체공학회:학술대회논문집
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• 한국전산유체공학회 2006년도 PARALLEL CFD 2006
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• pp.311-314
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• 2006

The supersonic flow around tandem cavities was investigated by three- dimensional numerical simulations using the Reynolds-Averaged Navier-Stokes(RANS) equation with the $\kappa-\omega$ thrbulence model. The flow around a cavity is characterized as unsteady flow because of the formation and dissipation of vortices due to the interaction between the freestream shear layer and cavity internal flow, the generation of shock and expansion waves, and the acoustic effect transmitted from wake flow to upstream. The upwind TVD scheme based on the flux vector split using van Leer's limiter was used as the numerical method. Numerical calculations were performed by the parallel processing with time discretizations carried out by the 4th-order Runge-Kutta method. The aspect ratio of cavities are 3 for the first cavity and 1 for the second cavity. The ratio of cavity interval to depth is 1. The ratio of cavity width to depth is 1 in the case of three dimensional flow. The Mach number and the Reynolds number were 1.5 and $4.5{\times}10^5$, respectively. The characteristics of the dominant frequency between two-dimensional and three-dimensional flows were compared, and the characteristics of the second cavity flow due to the fire cavity flow cavity flow was analyzed. Both two dimensional and three dimensional flow oscillations were in the 'shear layer mode', which is based on the feedback mechanism of Rossiter's formula. However, three dimensional flow was much less turbulent than two dimensional flow, depending on whether it could inflow and outflow laterally. The dominant frequencies of the two dimensional flow and three dimensional flows coincided with Rossiter's 2nd mode frequency. The another dominant frequency of the three dimensional flow corresponded to Rossiter's 1st mode frequency.

• 한국항공우주학회지
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• 제32권9호
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• pp.27-34
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• 2004

측 추력(Lateral Jet) 제어 시스템에 의해 자세제어를 하는 미사일 주위의 초음속 유동장 해석을 위하여 삼차원 Navier-Stokes 코드 (AADL3D)를 개발하고, 이를 이용한 수치해석 연구를 수행하였다. 미사일의 받음각, 제트 노즐의 위치, 그리고 제트의 분출 각 등의 Parameter가 미사일에 미치는 수직력 및 피칭모멘트에 대한 영향을 알아보기 위한 사례 연구를 수행하였다. 또한 미사일은 무게 중심을 기준으로 4개 영역으로 나뉘어 각 부분에서의 수직력과 모멘트에 대한 기여도를 비교하였다. 공력해석 결과, 각 Parameter 변화에 대한 서로 다른 수직력과 모멘트 변화양상 및 그 원인을 확인할 수 있었다. 또한 각 Parameter 의 적절한 조합에 의해 모멘트 발생을 최소화 할 수 있음을 보여 주었다.

• 한국공간정보시스템학회 논문지
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• 제11권4호
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• pp.56-64
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• 2009

최근 웹 2.0 기술의 활용이 증가하면서 RIA (Rich Internet Application) 기술에 대한 중요성도 증가하고 있다. RIA는 인터넷 서비스가 가능한 데스크탑 및 모바일 기기에서 다양한 정보를 제공할 수 있는 장점이 있다. 본 논문에서는 RIA 기술 중에서 플래시를 사용하여 공간 데이터를 모바일 환경에서 서비스하는 방법을 제안한다. 공간 데이터 서버는 사용자가 요구한 공간 데이터를 RIA 기술 중 하나인 플래시 기반의 웹 어플리케이션에 포함하여 제공하는 방법을 사용한다. 본 논문에서 제안하는 방법은 클라이언트에서 렌더링 및 사용자 인터페이스 처리를 담당하는 특징을 가진다. 또한, 서버로부터 웹 어플리케이션을 다운로드 받으면 추가로 공간 데이터 서버에 접속 없이도 클라이언트 자체에서 공간 데이터의 패닝, 확대/축소 등의 처리가 가능하므로 무선 언터넷 환경을 사용하는 모바일 장치에서 효과적이다. 그리고, 풀랫폼에 독립적으로 동작되어 모바일 환경에서도 데스크탑 환경과 동일하게 활용할 수 있는 장점이 있다. 본 논문에서 제안하는 공간 데이터 서버의 성능을 평가하기 위하여 WMS(Web Map Server)와 비교 분석한다.

• 한국추진공학회지
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• 제6권1호
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• pp.12-20
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• 2002

케로신/액체산소 추진기관을 갖는 KSR-III 로켓의 플룸 유동장에 대하여 로켓 동체/플룸 유동장에 대한 통합적인 해석을 수행하였다. 기체 열-화학 모델이 유동장에 미치는 영향을 평가하여 로켓 유동장을 해석하는 목적에 가장 적합한 기체 모델을 제시하기 위하여 열량적 완전기체, 다윈 화학종 반응기체, 그리고 화학적 동결기체의 세 가지 기체 모델을 사용하여 유동장을 해석하고 그 차이를 검토하였다. 반응유동 해석 결과는 노즐 내부에서의 화학반응에 의한 연소가스의 온도 증가로 인해 다른 기체 열화학 모델에 비해 전체적으로 더 높은 온도 분포를 나타내었다. 플룸에서의 모든 화학반응은 전단류와 배럴 충격파 반사지점 후방의 고온 영역에 국한되어 일어났으며, 본 해석의 경우 플룸 내에서의 유한속도 화학반응이 유동에 미치는 영향은 미약한 것으로 나타났다. 그러나 본 연구에서 이루어진 유한속도 화학반응을 고려한 플룸 해석을 통하여 플룸에서의 주된 화학반응 및 반응 메커니즘을 확인할 수 있었다.

• 한국추진공학회지
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• 제5권1호
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• pp.26-33
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• 2001

제트베인 추력편향장치는 노즐 뒤에 장착되어 노즐에서 분사되는 초음속 제트의 유동방향을 편향시킴으로써 하나의 노즐로 피치, 요, 롤 방향의 제어를 할 수 있는 장치이다. 제어력을 얻기 위해 초음속 유동중에 노출되어 있는 제트베인에는 열 및 공기역학적 하중이 작용하게 되며, 제트베인의 형상 및 편향각에 따라 나타나는 충격파 및 제트베인 상호 유동간섭으로 인해 비행 추력 손실 및 측력의 크기에 영향을 미치게 된다. 본 연구에서는 마하 2.88 노즐 중에 놓인 제트베인의 피치 및 요, 롤 방향의 특성을 규명하기 위해 6 종의 제트베인을 선정하고, 각 방향에 따른 제트베인 편향각 $0^{\cire}$~$25^{\cire}$ 범위에서 $5^{\cire}$ 간격으로 유동시험을 각각 수행하였다. 또한, 유동해석을 병행하여 제트베인간의 유동 간섭 특성을 분석하였다. 연구 결과 제트베인간의 상호간섭은 나타나지 않으며, 제트베인의 공기역학적 특성은 현과 리드의 길이 비에 크게 좌우되고, 최대 추력손실은 롤 제어시 축추력의 17%로 나타났다.

• 한국추진공학회:학술대회논문집
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• 한국추진공학회 2004년도 제22회 춘계학술대회논문집
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• pp.165-172
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• 2004

LE-7A is the main engine of the H-IIA launch vehicle. Under its development, the nozzle suffered from two troubles during startup and shutdown transients of the engine. One is a large side load, which damages the actuator of the nozzle, and the other is damage on regenerative cooling tubes due to high heat load. It has been considered that these problems are caused by a peculiar separation pattern called Restricted Shock Separation (RSS). RSS is observed in several rocket nozzles, for example, LE-7A nozzle, Vulcain nozzle and so on. Their contours are not conventional truncated perfect (TP) nozzle - LE-7A nozzle is a compressed truncated perfect (CTP) nozzle and Vulcain nozzle is a thrust optimized (TO) nozzle. Although it is believed that the occurrence of RSS is affected by the nozzle contour, the mechanisms are not clarified sufficiently yet. In the present paper, a parametric numerical study is carried out to investigate the mechanisms of the occurrence of RSS in CTP nozzles during startup transient. The results show that RSS is caused by the adverse pressure gradient downstream of the Mach disk. The adverse pressure gradient is caused by the interaction of the pressure wave and Mach disk. The method to avoid the occurrence of RSS is also examined. A small step inside the nozzle affects the position of the separation point and prevents RSS. The result shows that the possibility that RSS can be suppressed by controlling the position of the separation point.

• Molecules and Cells
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• 제38권2호
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• pp.187-194
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• 2015

Thioredoxin (TRX) is a disulfide reductase present ubiquitously in all taxa and plays an important role as a regulator of cellular redox state. Recently, a redox-independent, chaperone function has also been reported for some thioredoxins. We previously identified nodulin-35, the subunit of soybean uricase, as an interacting target of a cytosolic soybean thioredoxin, GmTRX. Here we report the further characterization of the interaction, which turns out to be independent of the disulfide reductase function and results in the co-localization of GmTRX and nodulin-35 in peroxisomes, suggesting a possible function of GmTRX in peroxisomes. In addition, the chaperone function of GmTRX was demonstrated in in vitro molecular chaperone activity assays including the thermal denaturation assay and malate dehydrogenase aggregation assay. Our results demonstrate that the target of GmTRX is not only confined to the nodulin-35, but many other peroxisomal proteins, including catalase (AtCAT), transthyretin-like protein 1 (AtTTL1), and acyl-coenzyme A oxidase 4 (AtACX4), also interact with the GmTRX. Together with an increased uricase activity of nodulin-35 and reduced ROS accumulation observed in the presence of GmTRX in our results, especially under heat shock and oxidative stress conditions, it appears that GmTRX represents a novel thioredoxin that is co-localized to the peroxisomes, possibly providing functional integrity to peroxisomal proteins.

• Molecules and Cells
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• 제41권6호
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• pp.562-574
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• 2018

The tazarotene-induced gene 1 (TIG1) protein is a retinoidinducible growth regulator and is considered a tumor suppressor. Here, we show that DnaJ heat shock protein family member C8 (DNAJC8) is a TIG1 target that regulates glycolysis. Ectopic DNAJC8 expression induced the translocation of pyruvate kinase M2 (PKM2) into the nucleus, subsequently inducing glucose transporter 1 (GLUT1) expression to promote glucose uptake. Silencing either DNAJC8 or PKM2 alleviated the upregulation of GLUT1 expression and glucose uptake induced by ectopic DNAJC8 expression. TIG1 interacted with DNAJC8 in the cytosol, and this interaction completely blocked DNAJC8-mediated PKM2 translocation and inhibited glucose uptake. Furthermore, increased glycose uptake was observed in cells in which TIG1 was silenced. In conclusion, TIG1 acts as a pivotal repressor of DNAJC8 to enhance glucose uptake by partially regulating PKM2 translocation.