• 한국산학기술학회논문지
• /
• 제13권4호
• /
• pp.1822-1829
• /
• 2012

이 연구에서 DNS 모델의 정보처리모델을 자체 수정 보완하기 위해 정보순환모델을 개발하고 기존의 DNS 모델에서는 모의하지 못하는 부분을 모의할 수 있도록 수정 보완하였다. 개선된 정보순환모델이 DNS 모델의 정보처리모델보다 다양한 분야에 대해 모의/분석이 가능함을 보이고 이 연구가 향후 C4ISR 효과분석 모델의 국내 자체 개발을 위한 기반연구가 될 수 있을 것으로 기대한다.

• 천문학회보
• /
• 제46권1호
• /
• pp.28.2-28.2
• /
• 2021

We investigate the impact of ram pressure stripping due to the intracluster medium (ICM) on star-forming disk galaxies with a multiphase interstellar medium maintained by strong stellar feedback. We carry out radiation-hydrodynamic simulations of an isolated disk galaxy embedded in a 1011 M⦿ dark matter halo with various ICM winds mimicking the cluster outskirts (moderate) and the central environment (strong). We find that both star formation quenching and triggering occur in ram pressure-stripped galaxies, depending on the strength of the winds. HI and H2 in the outer galactic disk are significantly stripped in the presence of moderate winds, whereas turbulent pressure provides support against ram pressure in the central region, where star formation is active. Moderate ICM winds facilitate gas collapse, increasing the total star formation rates by ~40% when the wind is oriented face-on or by ~80% when it is edge-on. In contrast, strong winds rapidly blow away neutral and molecular hydrogen gas from the galaxy, suppressing star formation by a factor of 2 within ~200 Myr. Dense gas clumps with nH≳10 M⦿ pc-2 are easily identified in extraplanar regions, but no significant young stellar populations are found in such clumps. In our attempts to enhance radiative cooling by adopting a colder ICM of T=106K only a few additional stars are formed in the tail region, even if the amount of newly cooled gas increases by an order of magnitude.

• 천문학회보
• /
• 제44권2호
• /
• pp.47.2-47.2
• /
• 2019

Observations indicate that turbulence in molecular clouds of the interstellar medium (ISM) is highly supersonic (M >> 1) and strongly magnetized (β ≈ 0.1), while in the intracluster medium (ICM) it is subsonic (M <~1) and weakly magnetized (β ≈ 100). Here, M is the turbulent Mach number and β is the ratio of the gas to magnetic pressures. Although magnetohydrodynamic (MHD) turbulence in such environments has been previously studied through numerical simulations, some of its properties as well as its consequences are not yet fully described. In this talk, we report a study of MHD turbulence in molecular clouds and the ICM using a newly developed code based the high-order accurate, WENO (Weighted Essentially Non-Oscillatory) scheme. The simulation results using the WENO code are generally in agreement with those presented in the previous studies with, for instance, a TVD code (Porter et al. 2015 &, Park & Ryu 2019), but reveal more detailed structures on small scales. We here present and compare the properties of simulated turbulences with WENO and TVD codes, such as the spatial distribution of density, the density probability distribution functions, and the power spectra of kinetic and magnetic energies. We also describe the populations of MHD shocks and the energy dissipation at the shocks. Finally, we discuss the implications of this study on star formation processes in the ISM and shock dissipation in the ICM.

• 대한전자공학회논문지SP
• /
• 제43권5호
• /
• pp.30-36
• /
• 2006

변형된 면적기반영역선별 기법으로 문자영상 속에 내재되어 있던 영역 분할을 회복하는 새로운 기법을 제안한다. 정보영역과 바탕영역으로 양분되어 있는 이진 원영상에 비해 오염 및 훼손으로 관측영상은 얼룩점과 잡음이 전체 영상에 섞여 다수의 크고 작은 영역들이 혼재된 그레이스케일 형태가 된다. 이러한 영상을 종래의 문턱치 처리나 확률적 기법으로 영역 분할하려면 이진영상으로 전환시킴에 의한 영역 형태 변형 문제가 발생한다. 이 문제를 최소화하기 위해 마름모꼴 블록을 채택한 반복조건부양식(iterated conditional mode, ICM) 기법으로 이진 영상을 구현하여 일차적으로 영역들의 집합으로 분류하였다. 그 다음 현재고려중인 화소에서 화소의 영역형성 판별과 영역의 면적을 산출하였다. 이를 전체 화소에 걸쳐 순차적으로 확산하여 해당영역들의 정보영역으로의 귀속 여부를 선택적으로 판정 분할함으로 정보영역 본래 형태를 복원하였다. 이 때 지정 영역들의 산출 면적들은 하나의 집합으로 배속 정렬되며 확률처리로 얻은 판별 파라미터 값에 의해 선별된다. 그레이스케일 탁본영상을 대상으로 종래의 문턱치 영역분할 기법과 ICM 기법도 함께 실험하였다. 그 결과 종래의 기법에 비해 우수한 영역분할 효과를 얻을 수 있었다.

• 천문학회보
• /
• 제37권1호
• /
• pp.41.1-41.1
• /
• 2012

Interactions between the galactic interstellar medium (ISM) and the intra cluster medium (ICM) are believed to be one of the main processes affecting galaxy evolution in cluster environments. The aim of our research is to study the molecular gas properties of a galaxy under the ICM pressure in the cluster environment. It has been well known that cluster galaxies are deficient in atomic hydrogen gas (HI gas) compared to their field counterparts and now there is much evidence that low density ISM is being removed by ram pressure due to ICM wind. Meanwhile, no significant molecular gas deficiency of the cluster galaxy population has been found yet they show overall lower star formation rate than galaxies in the field, and it is still puzzling how the star formation could decrease without stripping of dense molecular gas. To address this issue, we probe the detailed molecular gas properties of NGC 4402, located near the cluster center, as part of a study of four spiral galaxies in the Virgo Cluster. NGC 4402 is well known undergoing ram pressure stripping with a truncated HI disk($D_{HI}/D_{opt}$ - 0.75 and only 36% of HI gas compare to field galaxies of a similar size) and a disturbed gas morphology. Comparing the high resolution 12CO and 13CO data of NGC 4402 from the Sub Millimeter Array (SMA) with existing other wavelength data, we probe the spatial distribution and a physical condition of molecular gas under strong ICM pressure. We discuss the star formation activity might have been altered and hence how the global color of NGC4402 would change in the future.

• 한국환경보건학회지
• /
• 제24권2호
• /
• pp.126-133
• /
• 1998

Effects of B(a)P on preimplantation mouse embryos in vitro were studied. Preimplantation mouse embryos were exposed to a concentration of 0.3, 1, 3 and 10 $\mu$M B(a)P for 72 hrs. The toxicological effects of B(a)P were evaluated by morphological observation of embryos up to the blastocyst stage, and by measuring DNA, RNA and protein synthesis by radioactive precursor incorporation. At 1 $\mu$M B(a)P did not affect preimplantation development but interfered with hatching and ICM formation. Suppressing effect of ICM formation was dose dependent. At the eight cell stage, the developmental rate was decreased at above 3 $\mu$M of B(a)P. At the blastocyst stage, attachment and trophoblast outgrowth were diminished at the 10 $\mu$M of B(a)P and ICM formation was decreased at 1 $\mu$M of B(a)P. Inner cell number of blastocyst was decreased dose dependently. So, number of ICM was one of the most sensitive and toxicological end point. The RNA incorporation rate of 0.1 $\mu ^3$H-uridine was dosedependent and the protein incroporation of 0.5 $\mu Ci ^{35}$S-methionine showed a significant decrease after 48 hrs. But the DNA incorporation rate of methyl-$^3$H thymidine was not affected. Our results suggested that B(a)P did not affect the DNA replication but transcription was inhibited by dose dependent manner. There delay of development during the blastocyst stage was mainly due to the inhibition of RNA synthesis followed by protein synthesis.

• Restorative Dentistry and Endodontics
• /
• 제43권3호
• /
• pp.18.1-18.12
• /
• 2018

Objectives: This study compared the retention of BioAggregate (BA; Innovative BioCeramix) and mineral trioxide aggregate (MTA; Angelus) as coronal plugs after applying different intracanal medications (ICMs) used in regenerative endodontic. Materials and Methods: One-hundred human maxillary central incisors were used. The canals were enlarged to a diameter of 1.7 mm. Specimens were divided into 5 groups (n = 20) according to the ICM used: calcium hydroxide (CH), 2% chlorhexidine (CHX), triple-antibiotic paste (TAP), double-antibiotic paste (DAP), and no ICM (control; CON). After 3 weeks of application, ICMs were removed and BA or MTA were placed as the plug material (n = 10). The push-out bond strength and the mode of failure were assessed. The data were analyzed using 2-way analysis of variance, the Tukey's test, and the ${\chi}^2$ test; p values < 0.05 indicated statistical significance. Results: The type of ICM and the type of plug material significantly affected bond strength (p < 0.01). Regardless of the type of ICM, BA showed a lower bond strength than MTA (p < 0.05). For MTA, CH showed a higher bond strength than CON, TAP and DAP; CHX showed a higher bond strength than DAP (p < 0.01). For BA, CH showed a higher bond strength than DAP (p < 0.05). The mode of failure was predominantly cohesive for BA (p < 0.05). Conclusions: MTA may show better retention than BA. The mode of bond failure with BA can be predominantly cohesive. BA retention may be less affected by ICM type than MTA retention.

• 한국동물번식학회:학술대회논문집
• /
• 한국동물번식학회 2001년도 춘계학술발표대회
• /
• pp.20-20
• /
• 2001

It has been reported that cloning cattle is inefficient. One of the problems was placental abnormality, finally resulting in fetal mortality after transfer of nuclear transfer (NT) bovine embryos. This study was focused on the allocations of embryonic cells to the inner cell mass (ICM) or to the trophectoderm(TE) in NT bovine blastocysts. Somatic cells were derived from a Day 45 fetus of gestation, individually transferred into enucleated oocytes and developed to the blastocyst stage in vitro. Differential staining was used to assess the qualify of blastocysts derived from NT, IVF and in vivo. Development rate of NT embryos to blastocysts (25.0%, 41/164) was similar to that of IVF embryos (28.7%, 49/171). The total cell number of NT blastocysts (101.3$\pm$45.9) was not different compared with that of IVF embryos (107.9$\pm$34.2, P>0.05), but was lower than in vivo embryos (122.5$\pm$21.6, P<0.05). Ratio of ICM/total cells was higher in NT embryos (51.6$\pm$ 18.6%) than in IVF and in vivo embryos (42.3$\pm$ 15.3% and 34.9$\pm$8.9%, respectively) (P<0.05). Most IVF (56.8%, 25/44) and in vivo blastocysts(80.8%, 21/26) was distributed in the proportion of ICM/total cells ranging from 20 to 40% group. However, most NT blastocysts was biased in the 40-60%(34.1%, 15/44) and >60% (31.8%, 14/44) groups. Our findings suggest that placental abnormalities or early fetal losses in the present cloning system may be due to aberrant allocation of NT embryos to the ICM cells.

• 천문학논총
• /
• 제30권2호
• /
• pp.491-494
• /
• 2015

We present 12CO (2-1) data for four spiral galaxies (NGC 4330, NGC 4402, NGC 4522, NGC 4569) in the Virgo cluster that are undergoing different ram pressure stages. The goal is to probe the detailed molecular gas properties under strong intra-cluster medium (ICM) pressure using high-resolution millimeter data taken with the Submillimeter Array (SMA). Combining this with Institut de RadioAstronomie $Millim{\acute{e}}trique$ (IRAM) data, we also study spatially resolved temperature and density distributions of the molecular gas. Comparing with multi-wavelength data (optical, $H\small{I}$, UV, $H{\alpha}$), we discuss how molecular gas properties and star formation activity change when a galaxy experiences $H\small{I}$ stripping. This study suggests that ICM pressure can modify the physical and chemical properties of the molecular gas significantly even if stripping does not take place. We discuss how this affects the star formation rate and galaxy evolution in the cluster environment.

• 천문학회보
• /
• 제43권2호
• /
• pp.54.1-54.1
• /
• 2018

Recent observational studies suggest that the environmental effects can shape the evolution of galaxies in clusters. In an attempt to better understand this process, we perform idealized radiation-hydrodynamic simulations of RAM pressure stripping on star-forming galaxies using RAMSES-RT. We find that extended HI disks are easily stripped by moderate ICM winds, while there is no significant decrease in the total mass of molecular gas. RAM pressure tends to compress the molecular gas, leading to enhanced star formation especially when the gaseous disk is hit by edge-on winds. On the other hand, strong ICM winds that are expected to operate at the centre of clusters strip both HI and molecular gas from the galaxy. Interestingly, we find that the strong ICM winds can induce the formation of relatively dense (~1H/cc) HI gas clouds at a distance from the disk.