• The Journal of Korean Medicine Ophthalmology and Otolaryngology and Dermatology
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• v.10 no.1
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• pp.185-208
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• 1997

A Literatual Study on the external treatment of eye diseases, the result were as follows. 1. The external treatment of eye diseases used eyedrops(點,滴), steam bath(熏), washing(洗), plaster(敷). 2. Eyedrops used filterated decoction. 3. Eye diseases used Bomeolum(永片), Coptidis Rhiwma(黃連), Angelicae gigantis Radix(當歸) with clearing away heat and toxic materials, clearing away swelling, pain, ithing and convulsion, clearing away nebula 4. Eye diseases used B-1(晴明), B-2(찬竹), Tae-Yang(太陽), S-1(承泣), G-1(瞳子료), S-2(四白), TE-23(絲竹空), Eo-Yo(魚腰), G-14(陽白), Gu-Hu(球後), G-20(風池), B-18(肝兪), LI-4(合谷), Liv-3(太衡, B-23(腎兪), G-37(光明), Liv-2(行間), GV-23(上星), and S-36(足三里).

• Journal of The Korean Astronomical Society
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• v.38 no.3
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• pp.365-370
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• 2005

We have made a multi-wavelength study of the X-ray bright giant shell complex 30 Doradus in the Large Magellanic Cloud (LMC). This is the one of the largest H II complexes in the Local Group. The Australia Telescope Compact Array (ATCA) and the Parkes 64-m single dish observations reveal that the distribution and internal motions of H I gas show the effects of fast stellar winds and supernova blasts. The hot emitting gas within the 30 Doradus complex and the entire giant H II complex are encompassed by an expanding H I shell. We investigate the dynamical age of this H I shell and compare to the age of starbursts occurred in the 30 Doradus nebula using the radiative transfer model and the infrared properties.

• Publications of The Korean Astronomical Society
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• v.30 no.2
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• pp.159-161
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• 2015

We have carried out optical spectroscopic measurements of emission lines for a sample of Galactic planetary nebulae with Wolf-Rayet (WR) stars and weak emission-line stars (wels). The plasma diagnostics and elemental abundance analysis have been done using both collisionally excited lines (CELs) and optical recombination lines (ORLs). It was found that the abundance discrepancy factors ($ADF{\equiv}ORL/CEL$) are closely correlated with the difference between temperatures derived from forbidden lines and those from $He\;{\small{I}}$ recombination lines, implying the existence of H-deficient materials embedded in the nebula. The $H{\beta}$ surface brightness correlations suggest that they might be also related to the nebular evolution.

• The Bulletin of The Korean Astronomical Society
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• v.44 no.1
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• pp.85.2-85.2
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• 2019

We developed a new grid-based Monte Carlo code to trace far UV He II line photons that are incident on a thick H I region and subsequently transferred through Rayleigh and Raman scattering with atomic hydrogen. In particular, we consider a neutral region that is moving away from the He II emission source which is either monochromatic or is described by a Gaussian profile. The resultant Raman scattered He II line profiles from a monochromatic source are characterized by a double peaked core part with an extended Raman red tail that is attributed to multiple re-entry events. Complicated behaviors are observed in the case of a Gaussian He II source including the formation of a secondary red peak near the Balmer center dependent on the H I column density. A preliminary application of our results to the CFHT data of the planetary nebula IC 5117 is presented.

• The Bulletin of The Korean Astronomical Society
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• v.44 no.1
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• pp.48.3-48.3
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• 2019

We present analysis results of far infrared (IR) data for 3C 58. We use Herschel observations to measure the IR spectral slope of the source. Our measurements add new IR data points to exisiting high-frequency ones and allow us to improve the IR spectral energy distribution (SED) of 3C 58, and so a cooling break expected in the optical band can be located more precisely. We interpret the SED and the break using a synchrotron+ inverse-Compton model for PWNe and infer flow properties in 3C 58. Because the IR data are contaminated by foregrounds and backgrounds, we discuss impacts of the contamination on our conclusion.

• Proceedings of the Korea Information Processing Society Conference
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• 2010.11a
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• pp.906-908
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• 2010

클라우드 컴퓨팅 환경을 구축할 수 있게 하는 OpenNebula는 ONE 스케줄러를 통해 가상머신들의 라이프 사이클을 관리한다. ONE 스케줄러는 가상머신을 할당 할 때, 클러스터 노드의 물리적 자원 할당 여부만을 고려하기 때문에 가상 머신 생성 후의 부하를 예측하기 힘들다. 본 논문에서는 사용자의 이전 가상 머신 사용 패턴을 기반으로 부하 등급을 나누고 이 등급에 따라 가상머신을 동적으로 할당하는 기법을 제안한다.

• Proceedings of the Korea Information Processing Society Conference
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• 2009.11a
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• pp.125-126
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• 2009

본 논문에서는 클라우드 컴퓨팅 기반의 가상머신 임대 서비스 구현을 위해 OpenNebula 기반의 클라우드 클러스터를 구축하였다. 클라우드 클러스터는 1대의 Front-End와 4대의 클러스터 노드로 구성하고 클러스터 노드에는 Xen을 통하여 서버 가상화를 실현한다. 사용자는 개인 맞춤형 가상머신 요구사항 템플릿을 작성한 뒤 Front-End를 통하여 클라우드 클러스터에 가상 머신 임대 서비스를 요청한다. 본 실험에서 총18개의 가상머신을 임대하는 서비스를 실행하여 생성된 가상 머신의 동작 및 네트워크 서비스를 구현하였다.

• The Bulletin of The Korean Astronomical Society
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• v.45 no.1
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• pp.69.4-70
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• 2020

Raman-scattered He II features are known to be present in several young planetary nebulae (PNe) including NGC 7027, NGC 6302, IC 5117 and NGC 6790. These features provide a new spectroscopic window to probe both thick neutral regions and far UV regions near Lyman series. We carry out photoionization model calculations using 'CLOUDY' to explore He II emission strengths dependent on the physical conditions of the central star. The emission nebula is treated as a simple spherical shell with uniform density. It is found that detectable Raman-scattered He II are obtained for T∗ ~ 105 K in the presence of a thick neutral component. We present mock spectra exhibiting Raman He II features based on the photoionization calculations and compare them with observed data. We discuss effective strategies for searching young PNe with Raman-scattered He II emissivities.

• Publications of The Korean Astronomical Society
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• v.27 no.4
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• pp.259-260
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• 2012

Polycyclic aromatic hydrocarbons (PAHs) in Galactic planetary nebulae (PNe) are investigated by means of the unidentified infrared (UIR) bands. Continuous near- to mid-infrared spectra of PNe are obtained with the AKARI/IRC and the Spitzer/IRS. All 19 PNe in the present study show prominent dust emissions and we investigate the variation in the intensity ratios among the UIR bands. The ionization fraction and the size distribution of PAHs in PNe are derived using the UIR band ratios. We find that the ionization fraction of PAHs in PNe is around 0.0-0.6 and that small PAHs are scarce. The present result indicates a systematic trend of the $3.4{\mu}m$ aliphatic feature to become weak as the PAH ionization fraction increases.

• Journal of The Korean Astronomical Society
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• v.27 no.1
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• pp.31-44
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• 1994

The 4.8GHz formaldehyde absorption line in the dark clouds in M17 and NGC 2024 regions has been mapped. In both nebulae, we detected two $H_2CO$ line components. In M17, the 24km $S^{-1}$ cloud is closely associated with the HII region located in front of the radio continuum source, and the 19km $S^{-1}$ cloud is associated with the visual dark clouds with a larger extent which are closer to us. The 19km $S^{-1}$ cloud has a mass motion approaching to the HII region. In both clouds, a velocity gradient from the north-east to the south-west directions is observed. The linewidth has no variation indicating no collapsing motion. In NGC 2024, the 9km $S^{-1}$ feature is extended along the dark bar in front of the bright nebula and a weak second component at 13km $S^{-1}$ is confined to the immediate vicinity of the radio source. Indications are that the 9km $S^{-1}$ cloud is physically associated with the dark bar and the 13km $S^{-1}$ cloud is located behind the radio source. The angular extent, the column density, and the total mass of the clouds are derived. The radial velocities of other molecular lines observed in these clouds are compared.