• 천문학논총
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• 제25권4호
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• pp.113-118
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• 2010

The Henyey-Greenstein (H-G) phase function, which is characterized by a single parameter, has been generally used to approximate the realistic dust-scattering phase function in investigating scattering properties of the interstellar dust. Draine (2003) proposed a new analytic phase function with two parameters and showed that the realistic phase function is better represented by his phase function. If the H-G and Draine's phase functions are significantly different, using the H-G phase function in radiative transfer models may lead to wrong conclusions about the dust-scattering properties. Here, we investigate whether the H-G and Draine's phase functions would indeed produce significant differences in radiative transfer calculations for two simple configurations. For the uniformly distributed dust with an illuminating star at the center, no significant difference is found. However, up to ~ 20% of difference is found when the central star is surrounded by a spherical-shell dust medium and the radiation of $\lambda$ < $2000\;{\AA}$ is considered. It would mean that the investigation of dust-scattering properties using the H-G phase function may produce errors of up to ~ 20% depending on the geometry of dust medium and the radiation wavelength. This amount of uncertainty would be, however, unavoidable since the configurations of dust density and radiation sources are only approximately available.

• 천문학회보
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• 제37권2호
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• pp.140.2-140.2
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• 2012

The silicate carbon star IRAS 09425-6040 shows very conspicuous crystalline silicate dust features and excessive emission at far infrared. To investigate properties of dusty envelopes around the object, we use radiative transfer models for axisymmetric and sphericallly symmetric dust distributions. We perform model calculations for various possible combinations of dust shells and disks with various dust species. We compare the model results with the observed spectral energy distributions (SEDs) including the IRAS, ISO, AKARI, MSX and 2MASS data. We find that a model with multiple disks of amorphous and crystalline silicate and multiple spherical shells of carbon dust can reproduce the observed SED fairly well. This supports the scenario for the origin of silicate carbon stars that oxygen-rich material was shed by mass loss when the primary star was an M giant and the O-rich material is stored in a circumbinary disk. Highly (about 75 %) crystallized forsterite dust in the disk can reproduce the conspicuous crystalline features of the ISO observational data. This object looks to have a detached silicate and H2O ice shell with a much higher mass-loss rate. It could be a remnant of the chemical transition phase. The last phase of stellar winds of O-rich materials looks to be a superwind.

• Structural Engineering and Mechanics
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• 제68권5호
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• pp.527-536
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• 2018

The free vibration frequency responses of the graded flat and curved (cylindrical, spherical, hyperbolic and elliptical) panel structures investigated in this research considering the rectangular and tilted planforms under unlike temperature loading. For the numerical implementation purpose, a micromechanical model is prepared with the help of Voigt's methodology via the power-law type of material model. Additionally, to incur the exact material strength, the temperature-dependent properties of each constituent of the graded structure included due to unlike thermal environment. The deformation kinematics of the rectangular/tilted graded shallow curved panel structural is modeled via higher-order type of polynomial functions. The final form of the eigenvalue equation of the heated structure obtained via Hamilton's principle and simultaneously solved numerically using finite element steps. To show the solution accuracy, a series of comparison the results are compared with the published data. Some new results are exemplified to exhibit the significance of power-law index, shallowness ratio, aspect ratio and thickness ratio on the combined thermal eigen characteristics of the regular and tilted graded panel structure.

• 천문학회보
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• 제45권1호
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• pp.50.4-51
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• 2020

We report our discovery of Raman-scattered He II λ6545 feature in young planetary nebulae NGC 6886 and NGC 6881 which indicates the existence of atomic hydrogen components. Considering sharply increasing cross-section of hydrogen atom near the resonance, Raman-scattered He II features are a useful diagnostic tool to investigate the distribution and kinematics of H I region in planetary nebulae. The high-resolution spectroscopic observation was carried out using BOES installed on the 1.8 m telescope of BOAO. We estimate the column density of H I region and its expansion velocity using our grid-based Monte-Carlo radiative transfer code. We assume that the H I region is uniformly distributed in spherical shell geometry with an opening angle and expands with constant speed. Our best-fit model is shown with the column density NHI = 3 × 1020 cm-2 and expansion speed vexp = 25 km s-1 with the opening angle ~ 25° for NGC 6886, and NHI = 4 × 1020 cm-2 and vexp = 30 km s-1 with the opening angle ~ 35° for NGC 6881. We present brief discussions on the late-stage of evolution of stars with mass > 3 M⊙.

• Bulletin of the Korean Chemical Society
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• 제18권8호
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• pp.831-840
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• 1997

Core/shell structured composite metal oxides of Fe2O3/MgO were prepared by thermal decomposition of Fe(acac)3 adsorbed on the surface of MgO cores. The morphology of the composites conformed to that of the MgO used as the cores. Broad powder X-ray diffraction peaks shifted toward larger d, large BET surface area (∼350 m2/g), and the size of crystalline domains in nano range (4 nm), all corroborate to the nanocrystallinity of the Fe2O3/MgO composite which was prepared by using nanocrystalline MgO as the core. By use of microcrystalline MgO as the core, microcrystalline Fe2O3/MgO composite was prepared, and it had small BET surface area of less than 35 m2/g. AFM measurements on nanocrystalline Fe2O3/MgO showed a collection of spherical aggregates (∼80 nm dia) with a very rough surface. On the contrary, microcrystalline Fe2O3/MgO was a collection of plate-like flat crystallites with a smooth surface. The nitrogen adsorption-desorption behavior indicated that microcrystalline Fe2O3/MgO was nonporous, whereas nanocrystalline Fe2O3/MgO was mesoporous. Bimodal distribution of the pore size became unimodal as the layer of Fe2O3 was applied to nanocrystalline MgO. The macropores in a wide distribution which the nanocrystalline MgO had were absent in the nanocrystalline Fe2O3/MgO. The decomposition of CCl4 was largily enhanced by the overlayer of Fe2O3 on nanocrystalline MgO making the reaction between nanocrystalline Fe2O3/MgO and CCl4 be nearly stoichiometric. The reaction products were environmentally benign MgCl2 and CO2. Such an enhancement was not attainable with the microcrystalline samples. Even for the nanocrystalline MgO, the enhancement was not attained, if not with the Fe2O3 layer. Without the layer of Fe2O3, it was observed that the nanocrystalline domain of the MgO transformed into microcrystalline one as the decomposition of CCl4 proceeded on its surface. It appeared that the layer of Fe2O3 on the particles of nanocrystalline Fe2O3/MgO blocked the transformation of the nanocrystalline domain into microcrystalline one. Therefore, in order to attain stoichiometric reaction between CCl4 and Fe2O3/MgO core/shell structured composite metal oxide, the morphology of the core MgO has to be nanocrystalline, and also the nanocrystalline domains has to be sustained until the core was exhausted into MgCl2.

• 한국패류학회지
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• 제28권4호
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• pp.321-328
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• 2012

전라남도 완도군 인근연안에서 채집된 소라, Batillus cornutus의 혈구를 광학현미경과 전자현미경을 이용하여 혈구의 종류 및 미세구조적인 특징을 연구하였다. 광학현미경 상에서 소라의 혈구들은 호염기성 세포로 관찰되었다. 혈구의 형태학적인 특징으로 분류를 하였을 때 소라의 혈구는 모두 8종류로 나눌 수 있었다. 미성숙 혈구는 직경 약 4.5-5.5 ${\mu}m$로서 세포질 내에 지름 2-3 ${\mu}m$인 원형의 핵이 대부분을 차지하고 있었다. 과립세포는 직경 약 7 ${\mu}m$로서 세포질에는 전자밀도가 낮고 크기가 다양한 과립들과 미토콘드리아, 글리코겐 과립들이 관찰되었다. 초자세포는 핵의 크기 및 세포질에 존재하는 미세소관의 특징에 따라 6종류로 세분화 할 수 있었다. 초자세포 III은 라이소좀 및 글리코겐 과립의 형성이 미약하여 식세포의 기능 보다는 영양분의 흡수 및 운반 기능을 수행하는 것으로 판단되며, 특히 초자세포 VI은 형태가 불규칙한 아메바형으로 세포질에 글리코겐 과립의 분포가 높고, 이식포와 자식포가 분포하고 있었다. 따라서 이들 혈구들의 정확한 기능을 파악하기 위해서는 효소학적 및 면역학적 연구를 추가적으로 수행해야 할 것으로 판단된다.

• 청정기술
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• 제29권2호
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• pp.95-101
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• 2023

폐굴껍질을 원료로 vaterite 형 침강성 탄산칼슘 제조 실험을 하였다. 굴껍질을 800℃의 온도에서 산화칼슘이 주성분인 소성 굴껍질을 제조하였다. 이 굴껍질을 질산이나 염산 용액에 녹여 0.1 M 질산칼슘이나 염화칼슘 수용액을 만들고, 여러 실험 조건에서 0.1 M 탄산나트륨 수용액과 탄산화 반응을 시켰다. 실험 조건은 aspatic acid 첨가량, 반응온도, 교반속도, NH₄OH 첨가량, 반응시간, 용해 산 종류 등이다. XRD, SEM, Size 분석을 하고 vaterite 함유량을 계산하였다. 25℃, 600 rpm, aspatic acid 0.1몰/ 1몰 CaO과 2 cm³의 NH₄OH를 첨가한 최적 조건에서 1시간 반응에서 vaterite 함유량 95.9%의 구형의 침강성 탄산칼슘을 합성하였다. 평균 입경은 12.11 ㎛이었다. 고 vaterite 함유 탄산칼슘은 의료용, 식용, 잉크첨가제 등 고부가가치 탄산칼슘으로 활용된다.

• 분석과학
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• 제21권3호
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• pp.237-243
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• 2008

착체중합법과 sol-gel법을 이용하여 ZnO 나노입자 표면상에 $TiO_2$ 입자를 코팅한 나노 코아쉘 구조를 제조하였다. 착체중합법으로 제조된 ZnO 입자는 평균입도가 약 100 nm, sol-gel법으로 제조된 $TiO_2$ 입자는 10 nm 이하의 크기로 각각 구성되었다. $ZnO@TiO_2$ 나노 코아쉘 구조의 평균입도는 약 150 nm의 크기를 나타내었다. 착체중합법으로 제조된 구형의 ZnO 나노 입자는 콜로이드상의 $TiO_2$ 입자의 균일한 표면흡착으로 인해 착체중합법으로 제조된 ZnO 입자의 입자간 응집이 크게 제어되었다. ZnO와 $TiO_2$의 이종 입자간의 표면전하는 pH 7 근처의 중성 영역에서 iso-electric point (IEP)의 차이로 인하여 - 로 대전된 $TiO_2$와 + 로 대전된 ZnO 나노입자의 이종의 입자들이 쿨롱의 인력에 의해 서로간의 결합을 하게 되고, 결합을 이룬 $ZnO@TiO_2$ 나노 코아쉘 구조가 표면 전하가 zero가 되어 발생하게 된다.

• Steel and Composite Structures
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• 제26권2호
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• pp.125-137
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• 2018

In this work, the bending and free vibration analysis of multilayered plates and shells is presented by utilizing a new higher order shear deformation theory (HSDT). The proposed involves only four unknowns, which is even less than the first shear deformation theory (FSDT) and without requiring the shear correction coefficient. Unlike the conventional HSDTs, the present one presents a novel displacement field which incorporates undetermined integral variables. The equations of motion are derived by using the Hamilton's principle. These equations are then solved via Navier-type, closed form solutions. Bending and vibration results are found for cylindrical and spherical shells and plates for simply supported boundary conditions. Bending and vibration problems are treated as individual cases. Panels are subjected to sinusoidal, distributed and point loads. Results are presented for thick to thin as well as shallow and deep shells. The computed results are compared with the exact 3D elasticity theory and with several other conventional HSDTs. The proposed HSDT is found to be precise compared to other several existing ones for investigating the static and dynamic response of isotropic and multilayered composite shell and plate structures.

• Fibers and Polymers
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• 제3권1호
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• pp.8-13
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• 2002

The effect of block sequence on the self-assembly of ABC-type triblock copolymers in the ordered state is investigated using an isothermal-isobaric molecular dynamics simulation. The block sequence has an important effect ,on the ]norphology of ABC triblock copolymers. Different morphologies are observed depending on the block sequence as well as the block composition. The triblock copolymers with the volume fraction of 1 : 1 : 1 ($f_A$=$f_B$=$f_C$= 0.33) show the three phase and four layered lamellar structures irrespective of the block sequence. The $A_{32}$$B_{16}$$C_{32}$triblock copolymer with $f_B$=0.2 shows a morphology In which cylinders of midblock B are formed at the interface between A and C lamellae, whereas the morphology of triblock copolymer $B_{16}$$C_{32}$ $A_{32}$ and $C_{32}$ $A_{32}$ $B_{16}$ show a cylindrical core-shell structure and a lamellar type morphology, respectively. The $A_{20}$$B_{40}$$C_{20}$the triblock copolymer with the block B as a major component shows a tricontinuous structure, whereas both $B_{40}$$C_{20}$$A_{20}$ and $C_{20}$$A_{20}$$B_{40}$ triblock coolymers exhibit the lamellar structures. When the block B has larger volrome fraction with $f_B$=0.75, the matrix is composed of block B, and other two blocks A and C form spherical domains.