• 한국지역지리학회지
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• 제20권2호
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• pp.163-175
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• 2014

본 연구는 필리핀 출신 결혼이주여성의 사회자본 특성을 근린지구 수준에서 설명하고자 한다. 연구의 주 대상은 한국의 대도시와 중소도시, 촌락 등에 거주하는 필리핀 출신 결혼이주여성들이며 그들이 주로 참여하는 근린공동 체- 학교, 성당공동체-에서 생산되는 사회자본에 대한 인식을 측정하여 개인적 특성과 공동체의 특성(결속력, 동질성 등)에 따른 사회자본의 특성에 대해 파악하였다. 연구 결과 학교공동체와 성당공동체에서 이주자의 개인적 특성 가운데 이주사회에서의 거주기간과 사회자본 간 관련성에서 차이를 보이고 있는데, 성당공동체는 거주기간과 사회자본 '관계'요소 간 정(+)적인 유의미한 결과가 도출되어 이주 후 기간이 증가할수록 성당공동체에서의 관계가 향상되는 것으로 나타났으며 학교공동체에서는 거주기간과 사회자본 '신뢰'요소가 부(-)적인 관계를 보이고 있어 거주기간이 길수록 신뢰가 오히려 감소하는 것으로 나타났다. 동질 성과 결속력, 사회자본의 양에서도 성당공동체가 우위를 점하고 있으며 특히 사회자본 '관계'는 공동체의 동질성과 더 밀접하며 '규범'은 공동체의 결속력과 밀접하다는 결과를 보이고 있다. 두 공동체에서 모두 의사결정과 가치추구 공유 및 규칙 준수 등의 '규범' 요소가 구성원 간의 '관계'요소와 유사하며, 만족도와 정서적 도움 및 제도에 대한 구성원들의 '신뢰'가 개인문제를 토론하고 참여하는 '정치'와 근접한다는 공통된 경향이 나타나고 있다. 연구과정에서 주목되는 것은, 초국가적 행태가 발생하는 회로로서의 성당공동체의 상징성으로, 성당공동체는 필리핀 결혼이주여성들의 고유한 집단적 문화와 개인적 욕구가 사회자본의 생산과 맞물리는 영역으로 확인되었다. 이는 필리핀 결혼이주여성들의 공동체와 사회자본의 특성에서 이주자로서의 개인적 특성과 함께 필리핀 결혼이주여성이 집단적으로 보유하는 family reunion 등의 사회 문화적 특질이 주는 영향 또한 간과할 수 없음을 잘 보여주고 있다. 이러한 부분은 민족적 정체성을 바탕으로 한 공동체성과 사회자본이 우리 사회와의 상호문화성을 공유하고 실천할 수 있는 주요 통로가 될 수도 있다는 점에서 의미 있으며 나아가 '민족 단위의 공동체와 그 사회자본 연구'는 향후 더 다양한 공동체를 대상으로 다층의 공간 스케일로 확장, 연구되어야 할 필요가 있다.

• 미술이론과 현장
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• 제4호
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• pp.123-144
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• 2006

Foreigners who arrived in Korea after the age of enlightenment were Japanese, Chinese and 'Westerners' who were Europeans and Americans. The westerners were diplomats who visited Korea for colonization or for increasing their economical profits by trading after the spread of imperialism, and tourists curious of back countries, artists, explores and missionaries to perform their roles for their religious beliefs. They contacted with Korean cultural and educational people as missionaries and instructors during Japanese colonial period. In 1945, the allied forces occupied Korea under the name of takeover of Japanese colony after Japan's surrender and the relation between foreigners and Korean cultured men enter upon a new phase. For 3 years, American soldiers enforced lots of systems in Korea and many pro-American people were educated. This relationship lasted even after the establishment of the government of Korean Republic and especially, diplomats called as pro-Korean group came again after Korean War. Among them, there were lots of foreigners interested in cultures and arts. In particular, government officials under American Forces who were influential on political circles or diplomats widened their insights toward Korean cultural assets and collected them a lot. Those who were in Korea from the period of independence to 1950s wrote their impressions about Korean cultural assets on newspapers or journals after visiting contemporary Korean exhibitions. Among them, A. J. McTaggart, Richard Hertz and the Hendersons were dominant. They thought the artists had great interests in compromising and uniting the Orient and the West based on their knowledge of Korean cultural assets and they advised. However, it was different from Korean artist's point of view that the foreigners thought Korean art adhered oriental features and contained western contents. From foreigners' point of view, it is hard to understand the attitude Korean artists chose to keep their self-respect through experiencing the Korean war. It is difficult to distinguish their thought about Korean art based on their exotic taste from the Korean artists' local and peninsular features under Japanese imperialism. We can see their thought about Korean art and their viewpoint toward the third world, after staying in Korea for a short period and being a member of the first world. The basic thing was that they could see the potentialities through the worldwide, beautiful Korean cultural assets and they thought it was important to start with traditions. It is an evidence showing Korean artists' pride in regard to the art culture through experiencing the infringement of their country. By writing about illuminating Korean art from the third party's view, foreigners represented their thoughts through it that their economical, military superiority goes with their cultural superiority. The Korean artist's thought of emphasizing Korean history and traditions, reexamining and using it as an original creation may have been inspired by westerners' writings. 'The establishment of national art' that Korean artists gave emphasis then, didn't only affect one of the reactions toward external impact, 'the adhesion of tradition'. In the process of introducing Korean contemporary art and national treasure in America, different view caused by role differences-foreigner as selector and Korean as assistant-showed the fact evidently that the standard of beauty differed between them. By emphasizing that the basis to classify Korean cultural assets is different from the neighborhood China and Japan, they tried to reflect their understanding that the feature of Korean art is on speciality other than universality. And this make us understand that even when Korean artists profess modernism, they stress that the roots are on Korean and oriental tradition. It was obviously a different thought from foreigners' view on Korean art that Korean artists' conception of modernism and traditional roots are inherent in Korean history. In 1950s, after the independence, Korea had different ideas from foreigners that abstract was to be learned from the west. Korea was enduring tough times with their artists' self-respect which made them think that they can learn the method, but the spirit of abstract is in the orient.

• 천문학회지
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• 제24권2호
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• pp.217-271
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• 1991

We have observed dense core around young stellar objects, DR21, S140, Orion-KL, and L1551 using four millimeter-wave transitions of $HC_3N\;J$=4-3, J=5-4, J=10-9, and J=12-11. The spatial distribution of $HC_3N$ emission closely resembles the morphology of the previous CS observations that trace high density gas. These observations reveal the existence of $HC_3N$ dense cores around central IR source, elliptical in shape and almost perpendicular to the CO bipolar outflow axis. Small differences can be explained by that $HC_3N$ molecular line is more optically thin and is seen to be more detailed structure in the neighborhood of central IR sources. In S140 and Orion-KL, massive(${\sim}10\;M_{\odot}$), slowly rotating dense cores lie near at the central IR sources of bipolar outflows. The velocity channel maps of DR21 show that the bipolar outflow gas may have a correlation with the dense core of DR21. We analyzed intensities of the four lines to derive physical conditions in dense core from two methods, LTE and LVG. The column density of $HC_3N$, $N(HC_3N)$, between LTE and LVG calculations agree well with each other. The abundances of $HC_3N$ in each observing source have been estimated using the average values of $n(H_2)$ and $N(HC_3N)$ and assuming the size of dense core. The fractional $HC_3N$ abundances in massive dense cores of DR21, S140, and Orion-KL have a range of $(2-7){\times}10^{-10}$, while that of low mass dense core, L1551, has one order of magnitude greater value of $2{\times}10^{-9}$. This should be considered good agreement with the result by Morris et al.(1976). It may be considered that dense cores of DR21, S140, and Orion-KL may have almost same stage of chemical evolution, and their abundances have a small values relative to that of L1551. The column density $N(HC_3N)$ decreases with increasing distance from the densest part of the cloud, the central infrared source, and have the relation of $N(HC_3N){\varpropto}R^{\alpha}$, where a has a range of 0.65 to 0.89. The values of $n(H_2)$ are not varied with increasing distance from the dense core, and have almost same values. Therefore, it is considered that the dense cores in these regions probably consist of dense clumps in diffuse molecular gas medium, and $n(H_2)$ of each clump is ${\sim}10^5\;cm^{-3}$. Levels in the $T_{ex}$ increases with $n(H_2)$. It is considered that the $HC_3N$ dense cores are not completely thermalized. We examine the relationships between the luminosity of central infrared sources versus mass of the dense cores, and the luminosity of central infrared sources versus molecular hydrogen column density. Luminosities of the central IR sources show good correlation with mass and hydrogen column density of the dense core. Same has been found from CS observations. However, mass and size derived from $HC_3N$ observations are one order of magnitude smaller than those from CS. It can be interpreted that we see more central part of the cloud cores in $NC_3N$ lines than CS lines.