• 한국우주과학회:학술대회논문집(한국우주과학회보)
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• 한국우주과학회 2009년도 한국우주과학회보 제18권2호
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• pp.34.4-35
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• 2009

We have studied the radial g-r color gradients of early-type galaxies in the Sloan Digital Sky Survey (SDSS) DR6 in the redshift range 0.00 < z < 0.06. The color profiles of ~30 per cent of the galaxies in this sample show positive color gradients (centers being bluer). These positive gradient galaxies often show strong $H\beta$ absorption line strengths or emission line ratios that are consistent with star-forming populations. Combining the optical data with Galaxy Evolution Explorer (GALEX) UV photometry, we find that all positive gradient galaxies show blue UV-optical colors. They also exhibit a tendency of having a lower stellar velocity dispersion. Positive gradient galaxies tend to live in lower density regions than negative gradient galaxies and are likely to have a late-type companion galaxy. On the other hand, massive early-type galaxies show negative color gradients. A simplistic population analysis shows that these positive color gradients are visible only for half a billion years after a star burst. Although the effective radius decreases and mean surface brightness increases due to this centrally concentrated star formation, the positions of the positive gradient galaxies on the fundamental plane cannot be reproduced by any amount of recent star formation. Instead it required a lower velocity dispersion.

• Journal of Astronomy and Space Sciences
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• 제16권1호
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• pp.1-10
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• 1999

The archival long-slit spectra, covering the wavelength range 4050 ~ 5150 $\AA$, have been used to investigate the radial behavior of absorption line fea-tures (G4300, Fe4383, Ca4455, Fe4531, and $H{\beta}$) of an elliptical galaxy NGC 5846A. The heliocentric recession velocity of NGC 5846 has been derived as $1949{\pm}87\;kms^{-1}$. Fe absorption lines of NGC 5846A show significant radial gradients with the mean slope of $\Delta/Delta(r")=-0.863\pm0.202$. There is also a significant radial gradient of G band with a slope of $-1.109{\pm}0.098$. On the other hand, no radial gradients has been detected on the Ca4455 and $H{\beta}$ absorptions of NGC 5846A. A metallicity gradient, which is derived from the Fe line gradients, is similar to the abundance gradient predicted by Larson's (1975) dissipative models for the formation of elliptical galaxies. We also note that a galaxy-galaxy interaction could affect the line gradients of NGC 5864A.

• 한국결정성장학회지
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• 제18권3호
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• pp.122-124
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• 2008

The partial phase diagram of $NaNO_3$-NaCl system was investigated and the eutectic temperature was determined as $294.5^{\circ}C$. A typical rod eutectics of $NaNO_3$-4.56 wt%NaCl was directionally solidified. The results of interrod spacing, ${\lambda}_E$ as a function of growth velocity, V, were. obtained as ${\lambda}_E\;V^{0.39}\;=\;5.26$ (temperature gradient, $G_l\;=\;21.4^{\circ}C/mm$) and ${\lambda}_E\;V^{0.32}\;=\;5.45$ ($G_l\;=\;3.9^{\circ}C/mm$) and the exponent numbers of growth velocity were smaller than the theoretical value, 1/2. The sample rotation applied during directional solidification made the interrod spacing decrease slightly.

• 한국주조공학회지
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• 제17권6호
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• pp.545-551
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• 1997

14 cm length Al-15Cu-1Mg alloys have been directionally solidified in 3 mm diameter alumina tubes in a furnace moved with a constant velocity V=12 cm/hr under various furnace temperatures of 660, 710 and $760^{\circ}C$. By analysing the evolution of the temperature profiles along the alloy length during the solidification, the growth characteristics such as the position of the solid/liquid interface, the local growth velocity (R) and the temperature gradient at the solid/liquid interface (G) have been determined. The effects of the furnace temperature on the growth behavior have been investigated by the comparison of R and G values for each temperature. Under the furnace temperature of $760^{\circ}C$, steady state growth region was observed for the latter half of the growth period.

• 대한화장품학회지
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• 제31권2호
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• pp.135-140
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• 2005

본 연구는 고형상 에멀젼의 표면에서 일어나는 물리적 특성을 레올로지를 이용해 관찰해 보았다. 고형상 에멀젼이 전단변형에 따라 고상에서 액상으로의 전이시 전단속도가 큰 고형상 에멀젼의 경우 낮은 전단변형과 높은 전단변형에서 두 번의 전이구간을 보여주는 반면에 전단속도가 작은 고형상 에멀젼의 경우 높은 전단변형에서 전이구간이 한 번만 나타내는 것을 볼 수 있었다. 이는 고형상 에멀젼의 전단변형에 따른 표면의 물리적 특성이 중요한 요소로서 고형상 에멀젼의 구성요소에 따라 변화하게 된다. 유상과 수상으로 구성되어진 고형상 에멀젼에서 수상의 함량이 증가하게 되면 표면전이(surface transition) 구간이 점점줄어들다가 사라지는 것을 볼 수 있었으며, 유상과 분체로 구성되어진 고형상 에멀젼에서는 분체의 함량이 증가함에 따라 표면전이 구간이 점점 증가하는 것을 볼 수 있었다. 그리고 유상, 수상 그리고 분체로 이루어진 고형상 에멀젼에서는 분체의 함량이 증가함에 따라 표면전이 구간이 점점 줄어들다가 사라지는 것을 볼 수 있었다.

• Korean Chemical Engineering Research
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• 제48권2호
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• pp.198-204
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• 2010

가압순환유동층 적용을 위해 루프씰(loop-seal: 내경 0.10 m)을 갖는 고체재순환부(직경 0.10 m, 높이 2.25 m)에서 층 물질로 silica sand 입자($d_p=240{\mu}m$, ${\rho}_s=2582kg/m^3$)를 사용하여 시스템 압력 변화(0.10~0.71 MPa)에 따른 고체흐름 특성을 연구하였다. 루프씰을 통한 고체질량플럭스는 공기주입량이 증가할수록 선형적으로 증가하였고, 동일한 공기주입속도에 대해 시스템 압력이 증가할수록 증가하였다. downcomer 내 압력변이는 시스템 압력이 증가할수록 동일한 공기주입속도에 대해 증가하였고, 흐름 내 고체속도 및 기체 속도 또한 증가하였다. 고체질량플럭스로부터 downcomer 에서의 압력변이를 예측할 수 있는 상관관계식을 Transportation number와 Pressure drop number를 이용하여 제안하였다. 루프씰에서의 압력강하는 시스템 압력에 관계없이 고체질량플럭스가 증가할수록 증가하였다. 각각의 시스템 압력에서 공기주입속도 변화에 따른 고체질량플럭스 및 Transportation number를 예측할 수 있는 상관관계식을 제안하였다.

• 상하수도학회지
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• 제9권4호
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• pp.63-72
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• 1995

The mean velocity gradient, G, has been used as a principal design and operation parameter for flocculation unit. This paper questions that significance. The physical and qualitative meaning of collision efficiency factors of each transport mechanism (Brownian motion, fluid shear, and differential sedimentation) are reviewed. The overall collision frequency function is calculated by summing up the collision frequency function of each mechanism. In the collision of two particles of different size, a diagram showing the dominant region in which each mechanism is important is developed and the meaning of the diagram is discussed. The primary ramification of this curvilinear, heterodisperse approach is that G is found to be not nearly so important. Previous experimental work in which the role of G has been examined is reviewed in light of this finding.

• 한국전산유체공학회지
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• 제3권1호
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• pp.63-72
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• 1998

The numerical simulations of flowfield and pollutant dispersion over two-dimensional hills of various shapes are described. The Reynolds-averaged Wavier-Stokes equations and concentration diffusion equation based on the gradient diffusion theory have been applied to the atmospheric shear flow over the bell-shaped hills which are basic components of the complex terrain. The flow characteristics such as velocity profiles of the geophysical boundary layer, speed-up phenomena, mean pollutant concentration profiles are compared with experimental data to validate the present numerical procedure and it has been found that the present numerical results agree well with experiments and other numerical data. It has been also found that the distributions of ground level concentration are strongly influenced by the source location and height.

• 천문학회지
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• 제45권5호
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• pp.117-125
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• 2012

We present $^{12}CO$ J = 2-1 line observations of G54.1+0.3, a composite supernova remnant with a mid-infrared (MIR) loop surrounding the central pulsar wind nebula (PWN). We map an area of $12^{\prime}{\times}9^{\prime}$ around the PWN and its associated MIR loop. We confirm two velocity components that have been proposed to be possibly interacting with the PWN/MIR-loop; the +53 km $s^{-1}$ cloud, which appears in contact with the eastern boundary of the PWN and the +23 km $s^{-1}$ cloud, which has CO emission coincident with the MIR loop. However, we have not found a direct evidence for the interaction in either of these clouds. Instead, we detected an 5'-long arc-like cloud at +15-+23 km $s^{-1}$ with a systematic velocity gradient of ~3 km $s^{-1}$ $arcmin^{-1}$ and broad-line emitting CO gas with widths (FWHM) of ${\leq}7km\;s^{-1}$ in the western interior of the supernova remnant. We discuss their association with the supernova remnant.

• 한국세라믹학회지
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• 제32권3호
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• pp.341-348
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• 1995

An analysis of the use of temperature profiles in the determination of the kinetic parameters of combustion synthesis of Ti5Si3 were investigated. From profile analysis, an apparent activation energy of 12KJ/mol was calculated. The Maximum heating rate achieved during 10wt% Ti5Si3 reaction by the product dilution method was approximately $1.5\times$104 K/s. Coupling this value with the measured wave velocity of 7.02 cm/s yields a maximum thermal gradient of 2.14$\times$103 K/cm. The value of tr (=t*) was calculated to be 1.2$\times$10-1 s and the value of td (=tx) was calculated to be 32.89 s. Using the definition of t* and the measured wave velocity, the effective thermal diffusivity, $\alpha$, was calculated to be 0.59$\times$10 $\textrm{cm}^2$/s. From these analysis, the power function, G, was also calculated.