• 천문학회보
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• 제44권1호
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• pp.84.2-84.2
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• 2019

We present the absolute properties of the double-lined eclipsing binary KIC 6206751 exhibiting multiperiodic pulsations. The Kepler light curve of this system was simultaneously solved with the previously published radial-velocity data. The results indicate that the binary star is a short-period semi-detached system with fundamental parameters of $M_1=1.66{\pm}0.04M_{\odot}$, $M_2=0.215{\pm}0.006M_{\odot}$, $R_1=1.53{\pm}0.02R_{\odot}$, $R_2=1.33{\pm}0.02R_{\odot}$, $L_1=5.0{\pm}0.6L_{\odot}$, and $L_2=0.96{\pm}0.09L_{\odot}$. We applied multiple frequency analyses to the eclipse-subtracted light residuals and detected the 42 frequencies below $2.5days^{-1}$. Among these, three independent frequencies of $f_2$, $f_3$, and $f_4$ can be identified as high-order ($38{\leq}n{\leq}40$) low-degree (l=2) gravity-mode oscillations, whereas the other frequencies may be orbital harmonics and combination terms. The ratios between the orbital frequency and the pulsation frequencies are $f_{orb}:f_{2-4}{\simeq}2:3$, which implies that the ${\gamma}$ Dor pulsations of the detached primary star may be excited by the tidal interaction of the secondary companion. The short orbital period, and the low mass ratio and $M_2$ demonstrate that KIC 6206751 is an R CMa-type star, which is most likely evolving into an EL CVn star. Of seven well-studied R CMa-type stars, our program target is the only eclipsing binary with a ${\gamma}$ Dor pulsating component.

• 한국자기학회지
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• 제5권5호
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• pp.846-853
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• 1995

국소섭동을 포함하는 비대칭성 계의 전자구조 물성을 연구하기 위해서 밀접 결합 (tight-binding ; TB) linear-muffin-tin-orbital(LMTO) 방법과 회귀(recursion ; R) 방법을 결합한 실공간 전자구조 방법인 제일원리-자체충족적-스핀분극 TB-LMTO-R 방법을 개발하였다. 이 방법을 강자성 물질인 bcc Fe, hcp Co, fcc Ni등에 적용하여 송이의 크기, 회귀 계수, TB-LMTO Hamiltonian의 차수등을 변화시키며 국소 상태밀도와 자기 모멘트등의 수치적 수렴도를 고찰하였다. 송이 크기는 5,000개 원자 이상, 연속 분수 계수 n은 40이상, TB-LMTO Hamiltonian의 차수는 2차 이상이며 TB-LMTO-R 방법이 기존의 LMTO 방법의 결과와 거의 일치하는 결과를 준다는 사실을 얻었고 실공간 전자 구조 방법으로 TB-LMTO-R 방법의 충분한 신뢰도를 확인 하였다.

• 대한화학회지
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• 제23권5호
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• pp.286-295
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• 1979

非對稱으로 置環된 diene과 dienophile 間의 反應에서 配向性에 미치는 산촉매의 효과를 豫期하기 위해서 루이스酸과 錯物을 形成한 dienophile의 理論的모델에 FMO 理論을 적용하여CNDO/2 방법으로 고찰하였다. 電子的性質이 類似한 치환기로 치환된 diene, dienophile의 반응(즉, 電子不足 diene과 電子不足 dienophile의 반응)에서 일어나는 半極性 고리化반응을 제외한 주어진 대부분의 반응에 대해서, CNDO/2방법이 실험적인 配向性과 一致하는 좋은 결과를 주었다. 또한 二次軌道相互作用이 非對稱으로 치환된 diene과 dienophile의 Diels-Alder 반응의 배향성에 중요한 역할을 했다는 사실을 보여주었다. Anh의 방법이 다른 방법보다 수식적으로 간단할지라도, 非對稱전이상태를 강조한 Anh의 방법이 配向性 결정에 좋은 결과를 주었다.

• 한국산업융합학회 논문집
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• 제15권4호
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• pp.95-101
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• 2012

In order to explain observed catalytic reactivity of aminophosphine complexes (seven-membered chelate), total energy, net charge, atomic orbital electron population, HOMO and LUMO energy of free ligands are calculated by PM3 methods of HyperChem 6.0. Free ligands are 1,2-bis{(diphosphino)amino}propane{$H_2PNHCH_2CH(CH_3)NHPH_2$;ligand 1},1,2-bis{(dimenylphosphino)amino}propane{$(CH_3)_2PNHCH_2CH(CH_3)NHP(CH_3)_2$;ligand 2},1,2-bis{(diphenylphosphino)amino}propane{$(C_6H_5)_2PNHCH_2CH(CH_3)NHP(C_6H_5)_2$;ligand 3}. The result showed that ligand 3 is stable than ligand 2 and ligand 1 and ligand 2 is stable than ligand 1 in total energy. Net charge of P atom is changed by H atom, methyl groups and phenyl groups in P atoms. Net charge of N atoms in ligands is nagative. The results of atomic orbital electron population are similar net charge data..

• 한국진공학회:학술대회논문집
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• 한국진공학회 2015년도 제49회 하계 정기학술대회 초록집
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• pp.150.2-150.2
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• 2015

In this study, we analyzed the electric and optical characteristics by using various deposition rate ($0.5{\AA}$, $1.0{\AA}$ and $1.5{\AA}/s$) in order to enhance the performance in organic light-emitting devices (OLED). The organic multi-layer structures were deposited with NPB ($500{\AA}$ as hole transport layer), Alq3 ($600{\AA}$ as electron transport layer and emission layer) and LiF ($8{\AA}$ as electron injection layer) via SUNIC PLUS200 on Glass/ITO substrates. In this experiment, we examined the relationship between porous state of organic deposition and mobility of the organic materials. Among the three deposition rates, $0.5{\AA}/s$ achieved the highest performance of (10,786cd/m2, 4.387cd/A) comparing with that of $1{\AA}/s$ (7,779cd/m2, 3.281cd/A) and $1.5{\AA}/s$ (5,167cd/m2, 2.693cd/A). We confirmed that low deposition rate helps to arrange organic materials densely and to move easily another atomic location using inter-chain transporting by orbital overlap.

• Bulletin of the Korean Chemical Society
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• 제23권2호
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• pp.221-224
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• 2002

Nucleophilic addition reactions of benzylamines (BA; $XC_6H_4CH_2NH_2$) to ethyl-${\alpha}$-cyanocinnamates (ECC;$YC_6H_4CH$=C(CN)COOEt) have been investigated in acetonitrile at $30.0^{\circ}C$. The rate is first order with respect to BA and ECC. The rate is slower than that expected from the additive effect of ${\sigma}^-$ or $R^-$ for the activating groups (CN and COOEt). Natural. bond orbital ${\pi}^{\ast}_{c=c}$ calculations show that the contribution of COOEt group may not be fully effective despite the coplanar molecular structure. The selectivity parameters including the cross-interaction constant (${\rho}_{xy}$ = -0.22) indicate that the addition occurs in a single step. The kinetic isotope effects ($k_H/k_D$=2.5-2.8) involving deuterated BA ($XC_6H_4CH_2ND_2$) nucleophiles and activation parameters (${\Delta}H^{\neq}=4{\sim}6\;kcal\;mol^{-1};{\Delta}S^{\neq}=-45{\sim}-52\;e.u.$) suggest a cyclic transition state in which N-$C_{\alpha}$ and H-$C_{\beta}$ bonds are formed concurrently.

• Journal of Astronomy and Space Sciences
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• 제31권3호
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• pp.187-197
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• 2014

We have investigated the dynamical stability of the proposed companions orbiting the Algol type short-period eclipsing binary SW Lyncis (Kim et al. 2010). The two candidate companions are of stellar to substellar nature, and were inferred from timing measurements of the system's primary and secondary eclipses. We applied well-tested numerical techniques to accurately integrate the orbits of the two companions and to test for chaotic dynamical behavior. We carried out the stability analysis within a systematic parameter survey varying both the geometries and orientation of the orbits of the companions, as well as their masses. In all our numerical integrations we found that the proposed SW Lyn multi-body system is highly unstable on time-scales on the order of 1000 years. Our results cast doubt on the interpretation that the timing variations are caused by two companions. This work demonstrates that a straightforward dynamical analysis can help to test whether a best-fit companion-based model is a physically viable explanation for measured eclipse timing variations. We conclude that dynamical considerations reveal that the proposed SW Lyncis multi-body system most likely does not exist or the companions have significantly different orbital properties from those conjectured in Kim et al. (2010).

• 한국자기학회지
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• 제1권1호
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• pp.6-11
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• 1991

희토류금속과 천이금속의 화합물인 희토류 영구자석의 전기적, 자기적 성질등을 이해하고 자우리는 $SmCo_{5},\;NdB_{6},\;NdFe_{5},\;NdFe_{4}B$등의 비교적 간단한 희토류 화합물에 대한 자체충족적 전자구조 이론연구를 시도하였다. 국재 밀도함수 근사 LMTO(Linearized Muffin Tin Orbital)밴드 방법을 이용하여 $SmCo_{5}$ 영구자석을 포함한 희토류 금속 화학물의 기저상태의 물리적 파라미터들, 즉 에너지 밴드, 상태밀도, Stoner상수, 자기 모멘트 등을 구하여 이들의 전자기적 물성을 고찰하였다. Nd, Sm등의 희토류원소와 Fe, Co등의 천이원소, 또한 boron등의 원소들이 서로 금속 화합물을 형성할 때 일어나는 bonding효과, 즉 희토류금속의 f-전자와 d-전자, 천이금속의 d-전자, 또한 boron 금속의 s,p-전자와의 상호 작용, 그에 따른 전자구조, 자성의 변화에 대한 연구를 수행하였다.

• Journal of International Society for Simulation Surgery
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• 제3권2호
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• pp.77-79
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• 2016

Osteoma is one of the benign tumor that occurs on the bones all over the body. Mostly the simple excision is known to be enough. However, sometimes we encounter the troublesome situation where the osteoma is located in very challenging area, which results in the recurrence. 26 year female presented with the intractable intracranial osteoma. Given the disease entity of the osteoma, the simple excision would be enough or conservative management. But this osteoma turned out to be huge and recurrent in spite of the endoscopic resections, which causes the facial disappearance accompanied by the orbital vertical dystopia. Moreover, the patient's main concern was the pain. We performed the intracranial resection of the whole lesion and reconstructed the skull base and frontal bone as well as the part of the orbital wall. In order to restore the original bony anatomy, the 3D printing model was used based on the titanium mesh. I report this unusual case of the intractable intracranial huge osteoma. This report may be helpful for the other surgeons to make a decision on their similar cases in the future.

• Journal of Astronomy and Space Sciences
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• 제32권3호
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• pp.257-268
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• 2015

Characteristics of delta-V requirements for deploying an impactor from a mother-ship at different orbital altitudes are analyzed in order to prepare for a future lunar CubeSat impactor mission. A mother-ship is assumed to be orbiting the moon with a circular orbit at a 90 deg inclination and having 50, 100, 150, 200 km altitudes. Critical design parameters that are directly related to the success of the impactor mission are also analyzed including deploy directions, CubeSat flight time, impact velocity, and associated impact angles. Based on derived delta-V requirements, required thruster burn time and fuel mass are analyzed by adapting four different miniaturized commercial onboard thrusters currently developed for CubeSat applications. As a result, CubeSat impact trajectories as well as thruster burn characteristics deployed at different orbital altitudes are found to satisfy the mission objectives. It is concluded that thrust burn time should considered as the more critical design parameter than the required fuel mass when deducing the onboard propulsion system requirements. Results provided through this work will be helpful in further detailed system definition and design activities for future lunar missions with a CubeSat-based payload.