• 대한가정학회지
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• 제40권4호
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• pp.201-210
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• 2002

The purpose of this study was to extend the social teaming and imitation theory in an attempt to examine the effect of star-entertainer imitation behavior on clothing behaviors in relation to adolescents' age and gender variables. The research was a survey and the subjects were 895 adolescents in Taejon, Korea. The measuring instruments was serif-administrated questionnaire consisted of star-entertainer imitation behaviors and clothing behaviors. The collected data were analyzed using factor analysis, ANOVA, Duncan's multiple range test. Results were as fellows: 1) The results of analysing the response of star-entertainer imitation behaviors showed that adolescents had very positive attitudes and high psychological need to identify self with star-entertainers, however, their actual identification behaviors were not very noticeable because of parents' restraint and school regulations on students' appearances and clothing behaviors. 2) The results of analysing the response of clothing behaviors showed four factors such as 'fashion$.$clothing interest', 'psychological dependency on clothing' , 'clothing exhibition', and 'clothing conformity'. 3) Star-entertainer imitation behaviors had significant effects on clothing behaviors; the group with more star-entertainer imitation behaviors showed more fashion$.$clothing interest, higher psychological dependency on clothing and clothing exhibition, and lower clothing conformity than the group with less star-entertainer imitation behaviors. 4) Clothing behaviors showed the differences according as adolescents' age and gender; the female adolescents showed more fashion$.$clothing interest and clothing exhibition than male, the high school and cortege age groups showed higher psychological dependency on clothing than other age groups. It is concluded that the results of this study support social teaming and imitation theory since TV media give strong influence on the TV viewers through presenting various modeling stimuli to adolescents' lives.

• 천문학회보
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• 제40권1호
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• pp.47.2-47.2
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• 2015

At local, galaxy properties are well known to be clearly different in different environments. However, it is still an open question how this environment-dependent trend has been shaped. In this presentation, we will show the results of our investigation about the evolution of star-formation properties of galaxies over a wide redshift range, from z~2 to z~0.5, focusing its dependence on their stellar mass and environment. In the UKIDSS/UDS region, we estimated photometric redshifts and stellar population properties, such as stellar masses and star-formation rates, using the deep optical and near-infrared data available in this field. Then, we identified galaxy cluster candidates at z~0.5-2. Through the analysis and comparison of star-formation (SF) properties of galaxies in clusters and in field, we found interesting results regarding the evolution of SF properties of galaxies: (1) regardless of redshifts, stellar mass is a key parameter controlling quenching of star formation in galaxies; (2) At z<1, environmental effects become important at quenching star formation regardless of stellar mass of galaxies; and (3) However, the result of the environmental quenching is prominent only for low mass galaxies (M* < $10^{10}M_{\odot}$) since the star formation in most of high mass galaxies are already quenched at z > 1.

• 천문학논총
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• 제27권4호
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• pp.261-262
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• 2012

The aim of this research is to reveal the spatial distribution of the star formation activity of nearby galaxies by comparing CO molecular emission lines with the large area observation in far-infrared (FIR) lines. We report the imaging observations of NGC 253 by FIR forbidden lines via FIS-FTS and CO molecular lines from low to high excitation levels with ASTE, which are good tracers of star forming regions or photo-dissociation regions, especially spiral galaxies, in order to derive the information of the physical conditions of the ambient interstellar radiation fields. The combination of spatially resolved FIR and sub-mm data leads to the star formation efficiency within galaxy. The ratio between the FIR luminosity and molecular gas mass, $L_{FIR}/M_{H_2}$, is expected to be proportional to the number of stars formed in the galaxy per unit molecular gas mass and time. Moreover the FIR line ux shows current star formation activity directly. Furthermore these can be systematic and statistical data for star formation history and evolution of spiral galaxies.

• 한국언론정보학보
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• 제62권
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• pp.119-139
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• 2013

스타는 우리들의 삶과 무척이나 밀착해 있다. 이들이 만든 소비문화가 수용자대중의 의식에서부터 행동에 이르기까지 커다란 영향을 미치는 것만 보아도 그렇다. 스타의 경제적인 역할도 크다. 이들은 소비문화를 확산함으로써 기업들의 상품판매를 촉진하고, 이윤 실현을 돕는다. 더구나 스타는 사람들의 일상에 깊숙이 침투해 있다. 이렇게 스타들이 인기를 바탕으로 사람들의 일상적인 담론을 지배하는데 이런 힘을 두고 스타권력이라 한다. 이에 필자는 스타권력이 어떻게 형성되고, 어떻게 자본 축적에 기여하는지 조사했다. 이 연구는 3가지 연구 문제를 설정하여 스타권력의 자본주의적 성격을 규명하고자 했다. 이 글은 정치경제학을 분석의 틀로써 이용했다. 스타의 정치경제학이란 스타가 자본 증식에 기여하는 한편 지배이념을 확산하는 기능을 행태를 비판하는 학설이다. 논의 결과 스타권력은 경쟁을 통해 인기를 얻고 이에 기초하여 시장에 영향을 준다. 그럼으로써 스타권력은 수용자대중의 일상적 담론을 지배하는 힘을 가진다. 이것이 스타권력의 원천이다.

• 천문학회보
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• 제40권2호
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• pp.31.3-32
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• 2015

We present the physical properties of star forming regions in IC 10 obtained from Korea VLBI Network (KVN) 22GHz, the Submillimeter Array (SMA) CO, Very Large Array (VLA) HI 21cm, optical (U, B, V and H-alpha), and Spitzer infrared observations. IC 10 is a nearby (~0.7Mpc) irregular blue compact dwarf (BCD) galaxy which is likely to be experiencing an intense and recent burst of star formation. This nearby infant system showing high star formation rate but low metallicity (<20% of that of the Sun) provides critical environment of interstellar medium (ISM) under which current galactic star formation models are challenged. To make quantitative analysis of the ISM in the galaxy, we apply 2D cross-correlation technique to the multi-wavelength data for the first time. By cross-correlating different tracers of star formation, dust and gas phases in IC 10 in a two dimensional way, we discuss the gas properties and star formation history of the galaxy.

• 천문학회보
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• 제42권1호
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• pp.38.3-39
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• 2017

The N159 and N160 ionized regions in the Large Magellanic Cloud are an important extragalactic star-forming complex. The physical environments and the star formation stages are different in N159 and N160. We performed near-infrared polarimetry to those star forming regions with IRSF/SIRPOL 1.4-m telescope. Near-infrared polarization enabled us to trace the detailed structure of magnetic fields in star-forming regions. Through the polarimetric data of J, H, and Ks bands, we examined the magnetic field structures in the N159/N160 complex. In this presentation, we show complex distribution of the magnetic fields associated with dust and gas structures. We verify the local magnetic fields in each star-forming region, which appear to be related with local environments, such as interior and boundary of shell structure, star-forming HII regions, and boundaries between HII regions and dense dark clouds. We discuss the formation scenario of the N159/N160 complex suggested from the magnetic field structure.

• 복식
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• 제51권5호
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• pp.61-75
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• 2001

This study was intended to observe strategic fashion-presentation in Music stars according to the change of the star system in the Korean popular musics. The Korean Music stars since 1990s have been made, fabricated and have excessively depended on the demand of the teenagers. Therefore their distinctive fashion-presentation is considered as more important element than those of the past. Consequently. the characteristics of the fashion-presentation in the Korean Music star these days are as follows : First. Music stars shows fashion-presentation that has a consistent fashion theme. That is one of the key success factor to raise the recognition of star singer. Second. Music star produces fashion images which reflects identity and of subculture. Those appearance have won wild popularity of the Peeps 1990's new generation. Third. although there is no change music genre and emotion. through merely renovation of their fashion image, Music star got diversity and originality of the characteristics of contemporary cultural goods. Fourth. In case of famous dance groups, in the past they maintained a singular atmosphere as a group, but in 1990'Music star group each members of the group have individually fashion-presentation. So, they can get more fans. Fifth, Music singers borrow or duplicate fashion-presentation from each others. Such as similar fashion-presentation guarantees support of the same fans.

• 자원ㆍ환경경제연구
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• 제17권1호
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• pp.3-22
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• 2008

본 논문은 평활 전이 자기회귀모형(Smooth Transition Autoregressive Model : STAR)을 이용하여 우리나라 이산화탄소 배출량과 경제성장률 시계열의 비선형성과 주기적 행태에 대하여 설명한다. 비선형 검정 결과 이산화탄소 배출량과 경제성장률 시계열 모두 선형성을 기각하며, 주기적인 국면전환을 보이고 있다. 또한 STAR 모형에 근거한 비선형 그랜저 인과관계 검정에서는 선형의 검정 결과와 달리 이산화탄소 배출량과 경제성장률 시계열이 상호간에 유의적이고 강한 영향을 주고 있는 것으로 나타났다.

• 한국통신학회논문지
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• 제25권1A호
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• pp.1-9
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• 2000

이 논문에서는 덧셈형 백색 정규잡음과 동일채널 간섭 성분이 존재하는 마이크로셀 시스템에서 다양성 기법을 도입한 16 star-QAM은 위상 검차와 진폭 검사의 두단계로 분리되는 차동 검파 방식인데 이동 통신로상의 감쇄 때문에 성능이 떨어지는 것을 어느 정도 줄이고, 시스템의 복잡성도 줄일 수 있다. 그리고, 감쇄로 인해 성능이 떨어지는 것을 막기 위하여 위상 검파와 진폭 검파에 대해 각각 등이득 합성법과 최대비 합성법을 채택한 16 star-QAM의 성능을 라이스 계수{{{{ { K}_{ } }} }}, 최대 도플러 주시파 {{{{ { f}_{ } }} }}d{{{{ { T}_{ } }} }}, 신호대 동일채널 간섭파 전력비 그리고, 다양성의 가치 수 {{{{ { L}_{ } }} }}의 여러 가지 값에 대해 평가하였다.

• 대한전기학회:학술대회논문집
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• 대한전기학회 1994년도 하계학술대회 논문집 A
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• pp.66-68
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• 1994

강유전체 박막과 마이크로 가공기술을 이용하여 초전형 적외선 센서를 제작하였다. 초전형 적외선 센서는 $Pb_{1-x}La_xTi_{1-x/4}O_3$ (x=0.05) (PLT) 강유전체 박막 커패시터를 RF 마그네트론 스퍼터링 방식으로 백금 전극이 증착된 MgO 기판상에 결정 성장시킨 구조를 갖고 있다. 스퍼터링된 PLT 바닥은 높은 c-축 결정 구조를 가지므로 센서로 사용하기 위한 poling 처리 과정이 필요하다. 이는 적외선 이미지 센서를 구현함에 있어서 수율 향상에 필수적인 요소이다. 마이크로 가공 기술을 사용하여 센서의 열용량을 극소화 함으로서 센서의 효율을 최대화하였다. 제작된 센서의 상부에 폴리이미드를 코팅하고 MgO 기판을 선택적으로 식각하여 코팅된 폴리이미드가 강유전체 박막 커패시터를 지지하고 있는 구조를 구현하였다. 이렇게 제작된 센서의 감도는 상온에서 $8.5{\times}10^8cm{\cdot}{\sqrt}{Hz/W}$로 측정되었으며 이는 마이크로 가공 기술을 사공하지 않은 경우보다 약 100 때의 감도 향상을 가져왔다.