• 천문학회보
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• 제37권1호
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• pp.73.2-73.2
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• 2012

The far ultraviolet (FUV) wavelength (900-1750A) range includes a wealth of important astrophysical information related to the cooling of hot gas, fluorescent emission from H2 molecules, and starlight scattered off dust particles. Among these, we would like to focus on the scattered emission of the central star by dust with the example of the FUV halo surrounding ${\alpha}$ Vir (Spica). While scattering properties of dust have been studied with the GALEX data, the improved dataset of STSAT-1 revealed many detailed structures of this interesting region. For example, the FUV continuum map obtained from the STSAT-1 observations shows enhanced emission in the southern part of the Spica halo region, where the dust level is also high. In fact, the FUV continuum intensity is seen to have a good correlation with the IRAS 100${\mu}m$ emission data. It is also seen that the scattered spectrum is softer than the original one emitted by the central star, which is attributed to the increase in the dust-scattering albedo with wavelength. We have developed a Monte Carlo code that simulates dust scattering of light including multiple encounters. The code is applied to the present Spica halo region to obtain the scattering properties such as the albedo and the phase function asymmetry factor.

• 한국공간정보시스템학회:학술대회논문집
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• 한국공간정보시스템학회 2004년도 춘계 학술발표회 논문집 제1권1호(통권1호)
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• pp.75-82
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• 2004

Many researcher's efforts have made a significant advancement of space frame structure with various portion, and it becomes the most outsanding one of space structures. However, with the characteristics of thin and long term of spacing, the unstable behavior of space structure is shown by initial imperfection, erection procedure or joint, especially space frame structure represents more. This kind of unstable problem could not be set up clearly and there is a huge difference between theory and experiment. Moreover, the discrete structure such as space frame has more complex solution, this it is not easy to derive the formulation of design about space structure. In this space frame structure, the character of rise-span ratio or load mode is represented by the instability of space frame structure with initial imperfection, and snap-through or bifurcation might be the main phenomenon. Therefore, in this study, space frame structure which has a lot of aesthetic effect and profitable for large space covering single layer is dealt. And because that the unstable behavior due to variation of inner force resistance in the elastic range is very important collapse mechanism, I would like to investigate unstable character as a nonlinear behavior with a geometric nonlinear. In order to study the instability. I derive tangent stiffness matrix using finite element method and with displacement incremental method perform nonlinear analysis of unit space structure, star dome and 3-ring star dome considering rise-span $ratio(\mu}$ and load $ratio(R_L)$ for analyzing unstable phenomenon.

• 한국항해항만학회지
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• 제38권6호
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• pp.585-591
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• 2014

본 논문의 주 목적은 프루드 수가 0.5 이상인 중형 경비정의 속도성능을 모형시험 이전에 CFD 결과를 바탕으로 기존의 모형시험자료를 활용하였다. 모형시험 이전에 CFD를 이용하여 선속 별로 추정된 제동마력이 주어진 엔진마력을 만족하는지를 평가 하였다. 대상선박은 선미가 서로 다른 두 가지 선형을 선정하였다. 점성 유동장 계산은 상용 CFD 코드인 STAR-CCM+를 사용하였으며, 자유수면과 자세 변화(동적 트림)를 모두 고려하였다. 알몸 선체의 저항 값은 CFD를 이용하여 추정되었다. 점성 유동 해석을 통해 두 가지 선형의 자유수면 파형, 압력분포, 한계유선 그리고 프로펠러 면에서의 속도분포를 비교하였다. 점성 유동 해석 결과를 바탕으로 두 가지 선형에 대한 유효마력 즉, 저항성능을 평가하였다. 부가물 부착에 따른 저항 증가량과 준추진효율 계수(ETAD, ${\eta}_D$)는 모형시험 자료를 활용하였다. 중형 경비정과 같은 고속선박에 관한 속도성능 추정법이 CFD와 기존 시험자료를 이용하여 개발되었다.

• 한국콘텐츠학회논문지
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• 제15권6호
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• pp.487-498
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• 2015

본 연구는 호텔 직원의 감정노동이 육체적 정신적 스트레스 및 역할 외 행동과 어떠한 인과구조를 형성하는지 실증 분석함으로써, 인사관리 측면의 실무적 정보를 제공하고 육체적 스트레스에 관한 연구의 부재를 해소하는 것에 주목적을 두고 있다. 이를 위해 서울 시내 특1급 호텔 직원으로부터 264개의 표본을 추출하였으며, 주요 분석결과는 다음과 같다. 첫째, 감정노동의 표면적 행위는 육체적 정신적 스트레스에 정(+)의 영향을 미쳤으며, 내면적 행위는 정신적 스트레스에만 부(-)의 효과를 보일 뿐, 육체적 스트레스에는 유의하지 않았다. 둘째, 내면적 행위는 역할 외 행동에 정(+)의 영향력을 보인 반면, 표면적 행위의 효과는 유의미하지 않았다. 셋째, 정신적 스트레스는 역할 외 행동에 부(-)의 영향을 미치는 것으로 확인되었으며, 육체적 스트레스 또한 역할 외 행동에 유의한 효과를 나타냈다. 하지만 육체적 스트레스는 예상된 부(-)의 이론적 부호와는 달리 정(+)의 영향을 도출하였는데, 결론에서는 이러한 결과를 자기 보상 심리에 기초하여 논의하였다.

• 한국의상디자인학회지
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• 제8권1호
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• pp.127-136
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• 2006

These researches discussed promotions and effectiveness in the area of star marketing production, copying, advertising, and expenditure on clothes. The thesis is refreshing in the way it deals with analysis of strategical changes in the fashion of entertainers asia cultural industry developed. I specially focused on comparing and analyzing the changes in style of Hip Hop fashion from the period of inferior culture to the period in which their fashion is highly respected. Also, I'd like to study the influence of the fashion to Korean Hip Hop artists. The Hip Hop musicians developed their styles from underdog images of Hip Hop to glamourous and luxurious styles along with modeling in various magazines appealing sexually. In Korea, Seven and Hyori Lee are showing new and changed styles that are different from the past to their fans. The Hip Hop style now is showing with unimaginably luxurious styles as opposed to its original image. With their pursuance of ostentatious and luxurious styles Hip Hop was reborn as new Glam style. Old Hip Hop styles such as ripped jeans, safety pins, graffiti, and loose and exaggerated silhouette give inspirations to many worldly known designers and their collection. Hip Hop that used to be a branch of a low culture was able to grow to the culture of luxuries via the development the media and improvement of lives and the level of consciousness of the middleclass. Music stars with luxurious Hip Hop fashion influenced coming of a new musical genre and Korean musicians largely. I hope this research can help developing the unique low-culture and creating new trend in the field of entertainers' fashion.

• 천문학회지
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• 제39권4호
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• pp.107-114
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• 2006

We conducted an analysis of a selected region from the FCRAO $^{12}CO$ Outer Galaxy Survey. The selected region is located between galactic longitude $117^{\circ}$ and $124^{\circ}$ with the velocity of -23 km $s^{-1}. Molecular clouds in this region show a peculiar velocity field, protruding from the Local Arm population. The selected region is divided into 7 clouds by spatial location. Though we were not able to identify the direct driving source for peculiar velocity of our target region, we find that there are several internal YSOs or star forming activities; there are many associated sources like an outflows, a high-mass protostellar candidate and $H_2O$ maser sources. We attribute the driving energy source to older generation of episodic star formation. Masses of main clouds(cloud 1-4) estimated using a conversion factor from $^{12}CO$ luminosity are larger than $10^4M_{\odot}$. Other components have a small mass as about $10^3M_{\odot}$. Among main clouds, cloud 2 and 4 seem to be marginally gravitational bound systems as their ratio of $M_{CO}$ to $M_{VIR}$ is about $2{\sim}3$, and the internal velocity dispersion is larger than the centroid velocity dispersion. Total mass estimated using a conversion factor from $^{12}CO$ luminosity is $7.9{\times}10^4M_{\odot}$.

• 천문학회보
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• 제36권2호
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• pp.115.1-115.1
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• 2011

We analyzed the line profiles of the planetary nebula (PN) NGC 7009 secured with the Keck I HIES and BOES's spectral data. The 5 positions were taken over the nebular image, 4 points on the bright rim plus 1 point at the central position. The covered spectral wavelength range was $3250{\AA}-8725{\AA}$ in these observations. We decomposed the lines of HI, HeI, HeII, CII, NIII, [ClIII], [NII], [OII], [OIII], [SII], [SIII], [ClIII], and [ArIII] using the IRAF and StarLink/Dipso. After correcting the Earth's movement and the PN's radial velocities, -48.6 & -48.9 km/s, respectively, for the Keck & BOES, we produced the line profiles in a velocity scale. The zero velocity at each line profile clearly indicates which part of the components is approaching or receding, giving a general information of the kinematical structure. Almost all of the low-to-medium excitation lines, such as [NII], [SII], [O III], and [ArIII], secured at the central position and four positions along the major & minor axes, showed 3 components, double peak + a wide wing component, suggesting the fast outflow structures are present. The overall geometry is a prolate shell which also has a fainter outer shell in the halo zone, but there appears to be some peculiar sub-structures inside the main shell. The high excitation He I, HeII, NIII lines which might be formed close to the inner boundary of the shell show unusual features, completely different from the other lines. The HeII and these high excitation lines may be indicative of a relative recent fast outflow from the central star and the permitted lines such as NIII might be affected by the innermost structure. We discuss a possible presence of a jet-like fast outflow structure in an out-flow axis different from the main axis of the spheroid shell.

• 해양환경안전학회지
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• 제27권2호
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• pp.369-376
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• 2021

전 세계적으로 환경오염 문제로 국제해사기구인 IMO(International Maritime Organization)에서는 이산화탄소 배출량과 관련된 지수인 EEDI(Energy Efficiency Design Index)를 만들어 새로 건조되는 선박들에 대한 규제를 적용하고 있다. 본 연구에서는 158k 원유운반선의 선형과 프로펠러 후류를 분석하여 새로운 형태의 에너지 저감 장치인 ring stator를 제안하였다. 최근의 선박들은 반류가 적은 즉 선미부 유속이 빠른 경향으로 발전되고 있어 덕트가 포함된 ESD(Energy Saving Device)는 저속비대선이라도 컨테이너선처럼 적용하기가 어렵다. 본 연구에서 제안한 ring stator는 이러한 점을 고려하여 새로이 개발된 장치로써 자항 성능 향상 뿐 아니라 저항 성능의 최소화를 목표로 설계를 진행하였다. Star-CCM+의 상용 프로그램을 활용하여 CFD 해석을 통해 설계한 ring stator의 성능을 확인하였고 최종 제시한 설계안에 대해 약 3.4 %의 추진 효율 개선 효과가 있음을 확인하였다. 설계된 ring stator에 대한 실험과의 비교 등을 통해 성능 검증 및 보다 정도 높은 최적화에 대한 연구를 추후 수행할 계획이다.

• 천문학회보
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• 제46권1호
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• pp.55.2-56
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• 2021

The progenitor of Type Ia supernovae (SNe Ia) is mainly believed to be a close binary system of acarbon-oxygen white dwarf (CO WD) and non-degenerate companion (single degenerate) or another WD (double degenerate). However, it is unclear which system is more prevalent. Here, we present a high cadence optical/Near-IR light curve of normal but slightly faint type Ia SN 2019ein from IMSNG project. We fit the early light curve (t <+8.3 days from the first detection) with various models to find the shock-heated cooling emission from SN ejecta-companion interaction. No significant shock-heated cooling emission is found, from which we constrain the progenitor star size as the following. The upper limit (R_upper,*) of the companion size in R-band is ~0.2R_⊙ when forcing the first light time (t_fl) to have one value and ~0.9R_⊙ when using the mean value of tfl from the fitting in each band. Assuming the source of the I-band curve is almost powered from the radioactive decay, we obtained R_upper,*~1.2R_⊙. The early B-V color curve is in agreement with the model color curve of the 2M_⊙ main sequence companion. These results allow us to at least rule out large stars like red giants as a companion star of the binary progenitor system of this supernova. B-R and V-R color do not show any significant signs of a red bump, which shows a thin helium shell (MHe<0.1M_⊙) for the sub-Mch WD (double detonation model). In addition, we estimated the distance to NGC 5353 as 37.098±0.028Mpc.

• Journal of Gynecologic Oncology
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• 제29권6호
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• pp.93.1-93.11
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• 2018

The introduction of checkpoint inhibitors revolutionized immuno-oncology. The efficacy of traditional immunotherapeutics, like vaccines and immunostimulants was very limited due to persistent immune-escape strategies of cancer cells. Checkpoint inhibitors target these escape mechanisms and re-direct the immune system to anti-tumor toxicity. Phenomenal results have been reported in entities like melanoma, where no other therapy was able to demonstrate survival benefit, before the introduction of immunotherapeutics. The first experience in ovarian cancer (OC) was reported for nivolumab, a fully human anti-programmed cell death protein 1 (PD1) antibody, in 2015. While the data are extraordinary for a mono-immunotherapeutic agent and very promising, they do not match up to the revolutionary results in entities like melanoma. The key to exceptional treatment response in OC, could be the identification of the most immunogenic patients. We hypothyse that BRCA mutation could be a predictor of improved response in OC. The underlying DNA-repair-deficiancy should result in increased immunogenicity because of higher mutational load and more neoantigen presentation. This hypothesis was not tested to date and should be subject to future trials. The present article gives an overview of the immunologic background of checkpoint inhibition (CI). It presents current data on nivolumab and other checkpoint-inhibitors in solid tumors and OC specifically and depicts important topics in the management of this novel substance group, such as side effect control, diagnostic PD-1/programmed cell death-ligand 1 (PD-L1) expression assessment and management of pseudoprogression.