• 천문학회보
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• 제41권1호
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• pp.39.4-40
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• 2016

We aim to investigate formation of satellite sub-galactic structures around isolated dwarf galaxies using cosmological hydrodynamic zoom simulations. For this, we modify a cosmological hydrodynamic code, GADGET-3, in a way that includes gas cooling down to T~10K, gas heating by universal reionization when z < 8.9, UV shielding for high density regions of $n_{shield}$ > $0.014cm^{-3}$, star formation in the dense regions ($n_H$ > $100cm^{-3}$), and supernova feedback. To get good statistics, we perform three different simulations for different target galaxies of the same mass of ${\sim}10^{10}M_{sun}$. Each simulation starts in a cubic box of a side length of 1Mpc/h with 17 million particles from z = 49. The mass of dark matter (DM) and gas particle is $M_{DM}=4.1{\times}10^3M_{sun}$ and $M_{gas}=7.9{\times}10^2M_{sun}$, respectively, thus each satellite sub-galactic structure can be resolved with more than hundreds or thousands particles. We analyze total 90 sub-galactic structures that have formed outside of the main halos but infall the main halos. We found that 1) mini halos that interact more with the other mini halos tend to accrete the more mass, 2) mini halos that interact more before the reionization tend to form more stars, 3) mini halos with the more interaction tend to approach closer to the galactic center and have the lower orbital circularity, 4) survivals even in the strong tidal fields evolve baryon dominated system, such as globular clusters.

• ETRI Journal
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• 제37권3호
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• pp.450-459
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• 2015

Small cell networks, as an important evolution path for next-generation cellular networks, have drawn much attention. Different from the traditional base stations (BSs) always-on model, we proposed a BSs on-off model, where a new, simple expression for the probabilities of active BSs in a heterogeneous network is derived. This model is more suitable for application in practical networks. Based on this, we develop an analytical framework for the performance evaluation of small cell networks, adopting stochastic geometry theory. We derive the system coverage probability; average energy efficiency (AEE) and average uplink power consumption (AUPC) for different association strategies; maximum biased received power (MaBRP); and minimum association distance (MiAD). It is analytically shown that MaBRP is beneficial for coverage but will have some loss in energy saving. On the contrary, MiAD is not advocated from the point of coverage but is more energy efficient. The simulation results show that the use of range expansion in MaBRP helps to save energy but that this is not so in MiAD. Furthermore, we can achieve an optimal AEE by establishing an appropriate density of small cells.

• 천문학논총
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• 제30권2호
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• pp.447-449
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• 2015

Although the link between activity in the nuclei of galaxy and galactic mergers has been under scrutiny for several years, it is still unclear to what extent and for which populations of active galaxies merger-triggered activity is relevant. The environments of AGN allow an indirect probe of the past merger history and future merger probability of these systems, suffering less from sensitivity issues when extended to higher redshifts than traditional morphological studies of AGN host galaxies. Here we present results from our investigation of the environment of radio selected sources out to a redshift z=2. We employ the first data release J-band catalog of the new near-IR Infrared Medium-Deep Survey (IMS), 1.4 GHz radio data from the Faint Images of the Radio Sky at Twenty-cm (FIRST) survey and a deep dedicated VLA survey of the VIMOS field, covering a combined total of 20 sq. degrees. At a flux limit of the combined radio catalog of 0.1 mJy, we probe over 8 orders of magnitude of radio luminosity. Using the second closest neighbor density parameters, we test whether active galaxies inhabit denser environments. We find evidence for a sub-population of radio-selected AGN that reside in significantly overdense environments at small scales, although we do not find significant overdensities for the bulk of our sample. We show that radio-AGN in the most underdense environments have vigorous ongoing star formation. We interpret these results in terms of the triggering and fuelling mechanism of radio-AGN.

• 천문학회보
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• 제37권2호
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• pp.82.1-82.1
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• 2012

GRB100205A is a Gamma Ray Burst (GRB) which is suspected to be at redshift z=11-13 due to its very red H-K color($(H-K)_{vega}=2.1{\pm}0.5$). We observed a field centered at GRB100205A with Wide Field Camera (WFCAM) at United Kingdom Infrared Telescope (UKIRT) in Hawaii, in order to search a quasar that could be located around the GRB. The images were obtained in J, H, and K filters covering a square area of $0.78deg^2$. Our J-, H-, and K-band data reach the depths of 22.5, 22.1, and 21.0 mag (Vega) at $5{\sigma}$, respectively. Also using z-band image observed by CFHT, we find 8 candidates that have colors consistent with a quasar at z=11-13(non-detection in z-, J-band and $(H-K)_{vega}$ > 1.6). However, the shallow depths of J-, H-band are not enough to verify their true nature. Instead, we identify many red objects to be old or dusty galaxies at $z{\geq}3$. The number density of such objects appears about twice or more than that of the field of Cosmological Evolution Survey (COSMOS) and Ultra Deep Survey (UDS) of UKIRT Infrared deep sky survey (UKIDSS). On scales between 0.18' and 15' the correlation function is well described by a power law with an exponent of ${\approx}-0.9$ and this implies that those objects are like galaxies. It is interesting that many red galaxies exist in the region where the GRB was detected.

• 한국식품과학회지
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• 제35권2호
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• pp.297-301
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• 2003

동맥경화증과 같은 심혈관 질환을 야기시키는 주요 위험요인인 혈중 콜레스테롤의 수준을 낮추기 위하여 콜레스테롤 생합성 과정의 속도조절단계 효소의 하나인 squalene synthase의 활성을 저해하는 물질을 분리 정제하여, 물질의 이화학적 특성과 생물학적 특성을 검토하였다. Squalene synthase 저해물질은 acetone extraction, ethyl acetate extraction, silica gel column chromatography, sephadex LH-20 column chromatography, 결정화 등을 이용하여 분리 정제하여 YUF-01을 얻었다. 기기분석을 통하여 구조분석을 행한 결과 YUF-01은 분자량 368, 분자식 $C_{20}H_{21}O_6$으로 분석되었으며 243과 421 nm 에서 UV-VIS 흡광을 나타내었고 $^{13}C$ NMR spectrum과 $^1H$ NMR spectrum을 검토하였을 때 aromatic ketone 구조인 curcuminoid 계통의 curcumin과 일치하였다. Squalene synthase에 대한 curcumin의 $IC_{50}$ 값은 $100{\mu}M$이었으며, non-competitive inhibitor로 작용하였다.

• 한국산학기술학회논문지
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• 제9권6호
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• pp.1548-1554
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• 2008

은을 이용한 PMC (precious metal clay; 은점토)는 최근 신속한 조형이 가능하여 공예품의 제작용도로 시장이 확대되고 있다. 손으로 직접 조형되는 특성 때문에 PMC자체가 친환경적이어야 하며 소결온도에 따라 적정한 강도와 수축율이 보장되어야 한다. 이미 알려진 선진사의 PMC의 바인더와 달리, 팜오일, 글리콜릭산, 물을 주성분으로 한 새로운 바인더를 제안하여 새로운 PMC를 제안하고, 이를 이용하여 디스크형태의 시편을 성형하여 $700{\sim}900^{\circ}C$ ($50^{\circ}C$간격)구간에서 15분간 소결하여 이들의 경도, 무게변화, 수축률, 소결밀도, 미세구조변화 특성을 선진사의 PMC의 특성과 비교하였다. 제안된 PMC는 선진사의 것과 물성을 비교하여 조형용으로 사용 가능하다고 판단되었으며 $850^{\circ}C$-15분 조건이 조형물 제작에 유리한 소결 조건임을 확인하였다.

• 한국주조공학회지
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• 제40권4호
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• pp.118-127
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• 2020

Microstructural evolution during a heat treatment and high-temperature tensile properties have been investigated in conventionally cast CM247LC. In as-cast specimens, MC carbides with high amounts of Ta, Ti, Hf, and W were found to exist in the interdendritic regions, and γ' was observed in the form of cubes and octocubes prior to decomposition into cubes. In the heat-treated condition, some portion of eutectic γ-γ' remained, and uniform cubic γ' was observed in both interdendritic regions and dendrite core. Three types of carbides with different stoichiometries and compositions were found at the grain boundaries. MC carbides with high Hf contents were observed in the vicinity of eutectic γ-γ'. The highest tensile strength value was found at 750℃, whereas the greatest ductility appeared at 649℃. The effect of the temperature on the tensile properties was closely related to the dislocation structure. With increase in the test temperature, the density of dislocations inside γ' decreased, whereas that in the γ matrix increased. Stacking faults generated in γ' at 750℃ had a strengthening effect, whereas thermally activated dislocation motion at a high temperature was considered to have the opposite effect.

• 한국산학기술학회논문지
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• 제7권5호
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• pp.805-810
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• 2006

기존의 일반적인 주조공정에 의한 은제품 주얼리는 경도가 약해서 내구성이 떨어지고, 산화되기 쉬어서 표면색이 변하고, 주조공정 중에 발생한 표면 기공 잔류 등의 문제가 있었다. 이러한 기존 은 주얼리 제품의 결점을 해결하기 위해 92.5%Ag-6.5%Cu-1%Zn 조성을 가진 내식성이 강화된 소재에 일단 기존 주조공정으로 실린더형의 링을 만들고, 이 링에 일축 압력을 가하여 소성 변형시켜 표면경도와 표면기공의 저감 등 기존 공정의 단점들을 극복할 수 있는 신공정을 제안하였다. 주조된 실린더 링 시편에 일축방향의 힘으로 소성변형을 유발시키고 이 정도에 따른 시편의 비커스 경도와 밀도, 일축방향의 힘에 따른 미세구조 변화를 관찰하였다. 결과적으로 주어진 소성변형과 기계가공의 후속공정을 통하여 단순 주조 제품보다 그레인 사이즈가 50% 감소되어 경도가 2.3배 이상 향상되고 표면기공이 없는 은 합금 링 소재를 개발하였고. 이를 이용하여 기존 주조공정으로는 제작이 불가능하였던 텐션 스타일의 은합금 반지 제작에 성공하였다.

• Molecules and Cells
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• 제23권3호
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• pp.349-356
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• 2007

Simple Sequence Repeats (SSRs) represent short tandem duplications found within all eukaryotic organisms. To examine the distribution of SSRs in the genome of Brassica rapa ssp. pekinensis, SSRs from different genomic regions representing 17.7 Mb of genomic sequence were surveyed. SSRs appear more abundant in non-coding regions (86.6%) than in coding regions (13.4%). Comparison of SSR densities in different genomic regions demonstrated that SSR density was greatest within the 5'-flanking regions of the predicted genes. The proportion of different repeat motifs varied between genomic regions, with trinucleotide SSRs more prevalent in predicted coding regions, reflecting the codon structure in these regions. SSRs were also preferentially associated with gene-rich regions, with peri-centromeric heterochromatin SSRs mostly associated with retrotransposons. These results indicate that the distribution of SSRs in the genome is non-random. Comparison of SSR abundance between B. rapa and the closely related species Arabidopsis thaliana suggests a greater abundance of SSRs in B. rapa, which may be due to the proposed genome triplication. Our results provide a comprehensive view of SSR genomic distribution and evolution in Brassica for comparison with the sequenced genomes of A. thaliana and Oryza sativa.

• 한국소음진동공학회:학술대회논문집
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• 한국소음진동공학회 2000년도 추계학술대회논문집
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• pp.396-402
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• 2000

Porous structures of aluminum foam have been studied. The apparent foam shape, foam hight, density, pore size, shape, and their distributions in various section areas of the experimental samples have been investigated. The sample have been cast into metallic mold, using aluminum foam prepared from a precursor based on pure Al ingot mixed with various amount of 1-2wt% increasing viscosity and foam agent materials. The process provides for flexibility in design of foam structures via relatively easy control over the amount of hydrogen evolution and the drainage processes which occur during foam formation. This is facilitated by manupulating parameters such as the foaming agent, thermal histories during solidification and mix melt viscosities. The acoustical performance of the panel made with the foamed aluminum is considerably improved; its absorption coefficient shows NRC 0.6-0.8. It has been found that the Al foam is very preferable for the compactness of the thermal system.