• 천문학회보
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• 제40권1호
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• pp.59.1-59.1
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• 2015

We present hydrodynamic simulations of gas clouds that inflowing from the disk to a few hundred parsec region of the Milky Way. Realistic Galactic structures are included in our simulations by thousands of multipole expansions that describe 6.4 million stellar particles of a self-consistent Galaxy simulation (Baba, Saitoh & Wada, in prep.). We find that a hybrid multipole expansion model with two different basis sets and a thick disk correction well reproduces the overall structures of the Milky Way. We find that the nuclear ring evolves into 240 pc at T~1500 Myr, regardless of the initial size. For most of simulation runs, gas inflow rate to the nuclear region is equilibrated as ~0.02 Msun/yr, and thus accumulated gas mass and star formation activity is stabilized as $6{\times}10^7Msun$ and ~0.02M/yr, respectively. These stabilized values are in a good agreement with estimations for the CMZ. The nuclear ring is off-centered to the Galactic center by the lopsided central mass distribution of the Galaxy model, and thus an asymmetric mass distribution is arose accordingly. The lopsidedness also leads the nuclear ring to be tilted to the Galactic plane and to precess along the Galaxy rotation. In early evolutionary stage when gas clouds start to inflow and form the nuclear ring, the z-directional oscillations of the gas clouds results in the twisted, infinity-shaped nuclear ring. Since the infinity-shaped feature is transient only for first 100 Myr, the current infinity-shape observed in the CMZ may indicate that the CMZ forms quite recently.

• 천문학회지
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• 제46권1호
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• pp.33-40
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• 2013

We investigate the dependence of the extended X-ray emission from the halos of optically luminous early-type galaxies on the small-scale (the nearest neighbor distance) and large-scale (the average density inside the 20 nearest galaxies) environments. We cross-match the 3rd Data Release of the Second XMMNewton Serendipitous Source Catalog (2XMMi-DR3) to a volume-limited sample of the Sloan Digital Sky Survey (SDSS) Data Release 7 with $M_r$ < -19.5 and 0.020 < z < 0.085, and find 20 early-type galaxies that have extended X-ray detections. The X-ray luminosity of the galaxies is found to have a tighter correlation with the optical and near infrared luminosities when the galaxy is situated in the low large-scale density region than in the high large-scale density region. Furthermore, the X-ray to optical (r-band) luminosity ratio, $L_X/L_r$, shows a clear correlation with the distance to the nearest neighbor and with large-scale density environment only where the galaxies in pair interact hydrodynamically with seperations of $r_p$ < $r_{vir}$. These findings indicate that the galaxies in the high local density region have other mechanisms that are responsible for their halo X-ray luminosities than the current presence of a close encounter, or alternatively, in the high local density region the cooling time of the heated gas halo is longer than the typical time between the subsequent encounters.

• 한국응용곤충학회지
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• 제14권1호
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• pp.37-42
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• 1975

1) 이 조사에서 감악산 거미로 21과, 73속, 115종(7종미확정종 포함)을 확인하였고, 그 중 Trachelas japonicus 는 한국미기록속, 미기록종이며, (3) Dictyna sp. (W); (11) Episinus sp. (A) ; (76) Coelotes sp. (A); 는 각각 특징을 지니고 있으나 아직 종을 결정짓지 못했다. 2) 이 조사만으로 거미상을 결정지을 수는 없겠지만 대체적인 경향을 살핀다면, 전북계(Holarctic sp.)-5종$(4.6\%)$ 구북계 (Palaearctic sp.)-6종$(14.8\%$ 동양계 (Oriental sp.)- 5종 $(4.6\%)$이 되며, 한대종자 난대종의 비는 4 : 1로 되여 같은 위도인 내륙의 춘천지방과 저의 같은 비율을 나타내고 있다. 3) 중국대륙과의 공통종은 45종이었으며 $41.7\%$를 차지하고 있다. 4) 감악산의 거미상은 지리적으로 상당히 북쪽에 위치하고 있음에도 불구하고 저평성과 기온차가 적은 분지성등에 의해서 북방계의 특수종이 별로 없고, 난대종이 상당수진출하고 있다- 이를 한, 난대를 대표하는 주요 과의 종의 조성비로 살펴보면 한대성 : Lycosidae-3종 $(2.8\%)$ Linyphiidae-5종 $(4.2\%)$ 난대성 : Theridiidae-12종$(11.1\%)$ Argiopidae-32종$(20.4\%)$로 되여 난대성종이 31.5 : 7의 비로 우세하다.

• The Journal of Advanced Prosthodontics
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• 제3권2호
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• pp.81-84
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• 2011

PURPOSE. The aim of this in vitro study was to investigate the adhesion of initial colonizer, Streptococcus sanguis, on resin, titanium and zirconia under the same surface polishing condition. MATERIALS AND METHODS. Specimens were prepared from Z-250, cp-Ti and 3Y-TZP and polished with $1 {\mu}m$ diamond paste. After coating with saliva, each specimen was incubated with Streptococcus sanguis. Scanning electron microscope, crystal violet staining and measurement of fluorescence intensity resulting from resazurin reduction were performed for quantifying the bacterial adhesion. RESULTS. Surface of resin composite was significantly rougher than that of titanium and zirconia, although all tested specimens are classified as smooth. The resin specimens showed lower value of contact angle compared with titanium and zirconia specimens, and had hydrophilic surfaces. The result of scanning electron microscopy demonstrated that bound bacteria were more abundant on resin in comparison with titanium and zirconia. When total biofilm mass determined by crystal violet, absorbance value of resin was significantly higher than that of titanium or zirconia. The result of relative fluorescence intensities also demonstrated that the highest fluorescence intensity was found on the surface of resin. Absorbance value and fluorescence intensity on titanium was not significantly different from those on zirconia. CONCLUSION. Resin specimens showed the roughest surface and have a significantly higher susceptibility to adhere Streptococcus sanguis than titanium and zirconia when surfaces of each specimen were polished under same condition. There was no significant difference in bacteria adhesion between titanium and zirconia in vitro.

• 천문학회지
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• 제44권6호
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• pp.217-234
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• 2011

We present two large cosmological N-body simulations, called Horizon Run 2 (HR2) and Horizon Run 3 (HR3), made using $6000^3$ = 216 billions and $7210^3$ = 374 billion particles, spanning a volume of $(7.200\;h^{-1}Gpc)^3$ and $(10.815\;h^{-1}Gpc)^3$, respectively. These simulations improve on our previous Horizon Run 1 (HR1) up to a factor of 4.4 in volume, and range from 2600 to over 8800 times the volume of the Millennium Run. In addition, they achieve a considerably finer mass resolution, down to $1.25{\times}10^{11}h^{-1}M_{\odot}$, allowing to resolve galaxy-size halos with mean particle separations of $1.2h^{-1}$Mpc and $1.5h^{-1}$Mpc, respectively. We have measured the power spectrum, correlation function, mass function and basic halo properties with percent level accuracy, and verified that they correctly reproduce the CDM theoretical expectations, in excellent agreement with linear perturbation theory. Our unprecedentedly large-volume N-body simulations can be used for a variety of studies in cosmology and astrophysics, ranging from large-scale structure topology, baryon acoustic oscillations, dark energy and the characterization of the expansion history of the Universe, till galaxy formation science - in connection with the new SDSS-III. To this end, we made a total of 35 all-sky mock surveys along the past light cone out to z = 0.7 (8 from the HR2 and 27 from the HR3), to simulate the BOSS geometry. The simulations and mock surveys are already publicly available at http://astro.kias.re.kr/Horizon-Run23/.

• Asian Pacific Journal of Cancer Prevention
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• 제14권7호
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• pp.4161-4165
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• 2013

Objective: To investigate discriminating protein patterns and potential biomarkers in serum samples between pre/postoperative pancreatic cancer patients and healthy controls. Methods: 23 serum samples from PC patients (12 preoperative and 11 postoperative) and 76 from healthy controls were analyzed using matrix-assisted laser desorption and ionization time-of-flight mass spectrometry (MALDI-TOF MS) technique combined with magnetic beads-based weak cation-exchange chromatography (MB-WCX). ClinProTools software selected several markers that made a distinction between pancreatic cancer patients and healthy controls. Results: 49 m/z distinctive peaks were found among the three groups, of which 33 significant peaks with a P < 0.001 were detected. Two proteins could distinguish the preoperative pancreatic cancer patients from the healthy controls. About 15 proteins may be potential biomarkers in assessment of pancreatic cancer resection. Conclusion: MB-MALDI-TOF-MS method could generate serum peptidome profiles of pancreatic cancer and provide a new approach to identify potential biomarkers for diagnosis and prognosis of this malignancy.

• 천문학회보
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• 제41권1호
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• pp.35.3-36
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• 2016

We explore the role of bars in AGN-galaxy co-evolution using a volume-limited face-on late-type galaxy sample with $M_r$ < -19.5 and 0.02 < z < 0.055 selected from SDSS DR7. In this study, we investigate how $SFR_{fib}$ as a proxy of gas contents at galactic center (over 1~1.5 kpc bulge scale) and central stellar velocity dispersion, ${\sigma}$, of host galaxies are connected to the bar presence and AGN activity. We find that galaxies are distributed in three distinct regions over the $SFR_{fib}-{\sigma}$ space and the behaviors of their bar fraction ($f_{Bar}$) are clearly different for each region. Galaxies at the AGN dominant region tend to be gas-deficient as $f_{Bar}$ increases and bars are more frequently found in fully-quenched late-type galaxies at the quiescent region, suggesting that bars speed up of the consumption of gas by SF and lead a sudden decline in the central gas. Overall, the bar effects on the AGN activity are positive over the same space except for quiescent galaxies with ${\sigma}$ > $170km\;s^{-1}$. Most significant bar effect on the AGN activity occurs in the less massive galaxies having sufficient gas, whereas the effect on galaxies at the AGN dominant region with higher the AGN fraction is relatively small. We suggest that the bar affect both central SF and AGN activities, but differently for central gas amount and BH (or bulge) mass of galaxies. We also investigate the AGN-bar connection with only pure AGNs and then confirm that they give marginally the same results.

• 대한치과보존학회:학술대회논문집
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• 대한치과보존학회 2008년도 Spring Scientific Meeting(the 129th) of Korean Academy if Conservative Dentistry
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• pp.246-257
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• 2008

이 연구의 목적은 3차원 유한요소분석법을 사용하여 교합력의 위치와 방향이 상악 제2소구치의 치경부 복합레진 수복물의 응력분포에 미치는 영향에 대해 평가해 보고자 하였다. 발치된 상악 제2소구치를 이용하여 micro-CT (SkyScan1072; SkyScan, Aartselaar, Belgium)로 스캔한 후 HyperMesh Ver 6.0 (Altair Engineering, Inc., Troy, USA)와 3D-DOCTOR (Able Software Co., Lexington, MA, USA)로 3차원 유한요소 모형을 제작하였다. 제작된 소구치 모형에 쐐기형 와동을 형성하고 탄성계수가 서로 다른 혼합형 복합레진과 흐름성 복합레진으로 각각 수복하였다. 수복 후 설측교두의 협측사면 세 위치에 각각 수직, 20도, 40도의 각도로 하중을 가한 후 응력분포를 ANSYS Ver 9.0 (Swanson Analysis Systems. Inc., Houston, USA) 프로그램을 이용하여 인장 응력의 분포를 분석한 바 하중 위치와 관계없이 하중방향의 각도가 증가할수록, 또한 수복재료의 탄성 계수가 높을수록 인장응력도 증가하는 것으로 보아 교합력의 방향과 수복재료의 탄성계수가 치경부 수복물의 응력분포에 중요한 영향을 미치는 요소로 사료된다.

• Restorative Dentistry and Endodontics
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• 제33권3호
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• pp.246-257
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• 2008

이 연구의 목적은 3차원 유한요소분석법을 사용하여 교합력의 위치와 방향이 상악 제2소구치의 치경부 복합레진 수복물의 응력분포에 미치는 영향에 대해 평가해 보고자 하였다. 발치된 상악 제2소구치를 이용하여 micro-CT (SkyScan1072; SkyScan, Aartselaar, Belgium)로 스캔한 후 HyperMesh Ver 6.0 (Altair Engineering, Inc., Troy, USA)와 3D-DOCTOR (Able Software Co., Lexington, MA, USA)로 3차원 유한요소 모형을 제작하였다. 제작된 소구치 모형에 쐐기형 와동을 형성하고 탄성계수가 서로 다른 혼합형 복합레진과 흐름성 복합레진으로 각각 수복하였다. 수복 후 설측교두의 협측사면 세 위치에 각각 수직, 20도, 40도의 각도로 하중을 가한 후 응력분포를 ANSYS Ver. 9.0 (Swanson Analysis Systems. Inc., Houston, USA) 프로그램을 이용하여 인장 응력의 분포를 분석한 바 하중 위치와 관계없이 하중방향의 각도가 증가할수록, 또한 수복재료의 탄성계수가 높을수록 인장응력도 증가하는 것으로 보아 교합력의 방향과 수복재료의 탄성계수가 치경부 수복물의 응력분포에 중요한 영향을 미치는 요소로 사료된다.

• 대한소아치과학회지
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• 제29권3호
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• pp.389-396
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• 2002

이 연구의 목적은 전형적인 우식제거(bur)와 기계화학적으로 제거된 상아질($Carisolv^{TM}$)의 microtensile bonding strength를 비교하는 것이다. 다음과 같은 결합 system이 사용되었다; AB: All Bond 2(3M, USA), PB: Prime & Bond 2.1(Dentsply, DE), AQ: AQ Bond(sun medical, Japan). 교합면 우식증을 가지고 있는 42개의 사람 대구치를 6개 그룹으로 나누었다. 각각의 그룹은 다음과 같이 나누었다; $Carisolv^{TM}$를 적용한 그룹 A, B, C와 bur를 사용한 그룹 D, E, F, A와 D 그룹에서는 AB가 상아질 결합제로 사용하였고, 그룹 B, E는 PB를 그룹 C, F는 AQ를 사용하였다. 그 후 와동은 복합레진(Z-100)으로 충전하였다. 각각의 시편을 0.7 mm 두께로 자르고 0.7 mm의 넓이로 다시 잘랐다. Microtensile bonding strength test는 $0.5\;mm/min^{-1}$의 crosshead에서 시행하여 파절면을 scanning electron microscope(JSM-6400, Jeol, Japan)로 관찰하여 다음과 같은 결과를 얻었다. 1. $Carisolv^{TM}$로 우식을 제거했을 때 Microtensile bonding strength는 bur를 사용한 것에 비해서 75.8-80%로 감소하였다(p<0.05). 2. $Carisolv^{TM}$로 우식을 제거했을 때 Microtensile bonding strength가 감소된 정도는 상아질 결합제의 종류에 따라 각 군별로 차이가 없었다(p<0.05). 3. $Carisolv^{TM}$로 우식을 제거했을 때 All bonds는 32.6 MPa, Prime & bond는 30.1 Mpa, AQ bond는 21.2 Mpa이었다. 4. Bur와 $Carisolv^{TM}$로 우식제거시 AQ bond는 All bond와 Prime & bond 2.1보다 유의하게 낮은 결합강도를 가졌다(p<0.01).