• Bulletin of the Korean Chemical Society
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• 제25권1호
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• pp.101-105
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• 2004

The laser ablation/ionization time-of-flight mass spectrometry is applied to the isotopic analysis of solid samples using a home-made instrument. The technique is convenient for solid sample analysis due to the onestep process of vaporization and ionization of the samples. The analyzed samples were lead, cadmium, molybdenum, and ytterbium. To optimize the analytical conditions of the technique, several parameters, such as laser energy, laser wavelength, size of the laser beam on the samples surface, and high voltages applied on the ion source electrodes were varied. Low energy of laser light was necessary to obtain the optimal mass resolution of spectra. The 532 nm light generated mass spectra with the higher signal-to-noise ratio compared with the 355 nm light. The best mass resolution obtained in the present study is ~1,500 for the ytterbium.

• Journal of Astronomy and Space Sciences
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• 제26권1호
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• pp.1-8
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• 2009

질량비가 작은 접촉쌍성 FP Boo를 3색(B, V, R) CCD 측광관측하여 새로운 광도곡선을 얻었으며, Rucinski et al.(2005)의 시선속도곡선과 함께 Wilson-Devinney 프로그램에 적용하여 FP Boo의 새로운 측광학적 해와 절대물리량을 구하였다. FP Boo를 포함한 24개의 질량비가 작은 접촉쌍성의 H-R도로부터 FP Boo의 진화 상태도 일반적인 질량비가 작은 접촉쌍성의 진화 상태와 일치하는 위치에 놓이고 있음을 다시 확인하였다. 이번 관측을 통하여 얻은 우리의 광도곡선에서는 작지만 약간의 비대칭성을 보였다.

• 한국지하수토양환경학회:학술대회논문집
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• 한국지하수토양환경학회 2003년도 추계학술발표회
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• pp.144-147
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• 2003

In this study, the mass transfer behaviors of phenanthrene, anthracene, and pyrene in soil slurry reactor (SSR) using two-liquid phase (TLP) system were investigated. The mass transfer ratio and rate of PAH in the TLP system using light paraffine oil, which has the highest solubility of PAH, were influenced by the amount of light paraffine oil and mixing speed. When the amount of light paraffine oil decreased from 15 % to 2.5 % (v/v), the mass transfer ratio of anthracene decreased significantly compared with that of phenanthrene and pyrene. As mixing speed increased, the initial mass transfer rate of PAH within 1 day was enhanced. However, each final mass transfer ratio of three PAHs after 5 day was similar irrespective of mixing speed.

• 천문학회지
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• 제37권3호
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• pp.91-117
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• 2004

We analyze the dependence of the mass-to-light ratio of spiral galaxies on the present star formation rate (SFR), and find that galaxies with high present star formation rates have low mass-to-light ratios, presumably as a result of the enhanced luminosity. On this basis we argue that variations in the stellar content of galaxies result in a major source of intrinsic scatter in the Tully-Fisher relation (TF relation). Ideally one should use a 'population-corrected' luminosity. We have also analyzed the relation between the (maximum) luminous mass and rotational velocity, and find it to have a small scatter. We therefore propose that the physical basis of the Tully-Fisher relation lies in a relationship between the luminous mass and rotational velocity, in combination with a 'well-behaved' relation between luminous and dark matter. This implies that the Tully-Fisher relation is a combination of two independent relations: (i) a relation between luminosity and (luminous) mass, based mainly on the star formation history in galaxies, and (ii) a relation between mass and rotation velocity, which is the outcome of the process of galaxy formation. In addition to a 'population-corrected' Tully-Fisher relation, one may also use the relation between mass and luminosity, and the relation between luminous mass and rotation velocity as distance estimators.

• 천문학논총
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• 제30권2호
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• pp.385-387
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• 2015

Stellar mass is an important parameter of galaxies. We estimate the dynamical mass of an elliptical galaxy by its velocity dispersion and effective radius using the Hernquist model in the framework of MOdified Newtonian Dynamics (MOND). MOND is an alternative theory to the dark matter paradigm. In MOND the dynamical mass is the same as the baryonic mass or luminous mass, and in elliptical galaxies most of the baryons reside in stars. We select elliptical galaxies between redshift 0.05 and 0.5 from the main galaxy sample and the luminous red galaxy sample in the Sloan Digital Sky Survey. We find that the stellar mass-to-light ratio at different redshift epochs can be fitted by a gamma distribution, and its mean is smaller at smaller redshifts.

• 한국안전학회지
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• 제13권3호
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• pp.11-23
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• 1998

In this study, collapse test of thin-walled structure is performed under axially quasi-static and impact load in collapse characteristic to develop the optimum structural member for a light-oriented automobile. Furthermore, the energy-absorbing capacity is observed according to the variety of configuration(circular, square), aspect ratio in aluminum specimen to obtain basic data for the improved member of vehicle. In both quasi-static and impact collapse test, Al circular specimens collapse, in general, with axisymmetric mode in case of thin thickness while collapse with non-axisynmetric mode according to the thickness increase. For Al rectangular specimens, they collapse with axisymmetric mode in case of thin thickness, with mixed collapse mode according to the increase of thickness. In terms of initial max. load, Al square specimen turns out the best member among specimens, and then Al square, circular and circular with large scaling ratio, respectively. In case of quasi-static compression test, the absorbed energy per unit volume and mass shows higher in Al circular specimen, and then Al square, circular with large scaling ratio, respectively, according to shape ratio the absorbed energy per unit volume and mass in case of max. impact compression load is higher than that of static load. But the absorbed energy per unit volume and mass shows that Al circular specimen is the best member. Especially, unlike max. compression loan, the absorbed energy per unit volume and mass in impact test turns out the low value.

• Journal of Astronomy and Space Sciences
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• 제36권4호
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• pp.265-281
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• 2019

We present new BVRI light curves of UY UMa with no O'Connell effect and a flat bottom secondary eclipse. Light curve synthesis with the Wilson-Devinney code gives a new solution, which is quite different from the previous study: UY UMa is an A-subtype over-contact binary with a small mass ratio of q = 0.21, a high inclination of 81°.4, a small temperature difference of ΔT=18°, a large fill-out factor of f = 0.61, and a third light of approximately 10% of the total systemic light. The absolute dimensions were newly determined. Seventeen new times of minimum light have been calculated from our observations. The period study indicates that the orbital period has intricately varied in a secular period increase in which two cyclical terms with periods of 12^y.0 and 46^y.3 are superposed. The secular period increase was interpreted to be due to a conservative mass transfer of 2.68 × 10^-8 M_⊙/yr from the less massive to the more massive star. The cyclical components are discussed in terms of double-light time contributions from two additional bound stars. The statistical relations of Yang & Qian (2015) among the physical parameters of 45 deep, low mass ratio contact binaries were revisited by using the physical parameters of UY UMa and 25 Kepler contact binaries provided by Şenavci et al. (2016).

• 임산에너지
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• 제20권2호
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• pp.58-68
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• 2001

본 연구는 상대광도 차이에 따른 구상나무(Abies koreana Wilson) 유묘의 생장과 물질생산에 대하여 구명하고자 자연전광이 100, 50, 30, 10% 및 2%로 조절된 피음포지에서 구상나무 5년생 포트묘를 사용하여 24개월간 실시하였으며 다음과 같은 결과를 얻었다. 1. 3회의 수고생장을 측정한 결과, 가장 낮은 생장치를 기록한 2% 처리구를 제외하고 처리구 간에 큰 차이를 보이지 않았다. 2. 근원경생장은 상대광도가 낮아짐에 따라 단계적으로 감소하는 경향이 뚜렷하게 나타났다. 3. 상대적으로 낮은 광도에서 자란 유묘의 다음해 생장시작 시기가 늦어졌으며, 신엽의 갯수 및 신초의 갯수, 신초의 길이도 감소하였다. 4. 지상부와 지하부, 엽중량을 포함한 총 건물생산량은 광도가 감소할수록 점진적으로 감소하였다. 5. 구엽의 건물량에 대한 신엽의 건물량의 비율은 1년간 피음처리한 경우 0.99±0.25∼1.06±0.06으로서 100, 50, 30% 처리구에서 비슷하게 높았고, 10%와 2% 처리구에서 각각 0.60±0.04, 0.52±0.03으로서 그 비율이 상대적으로 낮았다. 2년간 피음처리한 경우에는 0.79±0.04∼1.00±0.03으로서 100, 50, 30, 10% 처리구에서 비슷하였고, 2% 처리구에서 0.29±0.03으로 매우 낮은 비율로 나타났다. 6. T/R율은 1년간 피음처리한 유묘의 경우 3.35±0.33∼4.61±0.25로서 100, 50, 30, 10% 처리구 간에 비슷하였으며, 2% 처리구에서는 7.36±0.15로서 다른 처리구에서보다 높게 나타났다. 2년간 피음처리한 유묘의 T/R율은 상대광도 2% 처리구의 2.01±0.14를 제외하고는 1.76±0.11∼3.12±0.19로서 상대광도가 감소할수록 높게 나타났다.

• Journal of Astronomy and Space Sciences
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• 제33권3호
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• pp.185-196
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• 2016

New multiband BVRI light curves of NSVS 1461538 were obtained as a byproduct during the photometric observations of our program star PV Cas for three years from 2011 to 2013. The light curves indicate characteristics of a typical W-subtype W UMa eclipsing system, displaying a flat bottom at primary eclipse and the O'Connell effect, rather than those of an Algol/b Lyrae eclipsing variable classified by the northern sky variability survey (NSVS). A total of 35 times of minimum lights were determined from our observations (20 timings) and the SuperWASP measurements (15 ones). A period study with all the timings shows that the orbital period may vary in a sinusoidal manner with a period of about 5.6 yr and a small semi-amplitude of about 0.008 day. The cyclical period variation can be interpreted as a light-time effect due to a tertiary body with a minimum mass of 0.71 M_⊙. Simultaneous analysis of the multiband light curves using the 2003 version of the Wilson-Devinney binary model shows that NSVS 1461538 is a genuine W-subtype W UMa contact binary with the hotter primary component being less massive and the system shows a low mass ratio of q(m_c/m_h)=3.51, a high orbital inclination of 88.7°, a moderate fill-out factor of 30 %, and a temperature difference of ΔT=412 K. The O'Connell effect can be similarly explained by cool spots on either the hotter primary star or the cool secondary star. A small third-light corresponding to about 5 % and 2 % of the total systemic light in the B and V bandpasses, respectively, supports the third-body hypothesis proposed by the period study. Preliminary absolute dimensions of the system were derived and used to look into its evolutionary status with other W UMa binaries in the mass-radius and mass-luminosity diagrams. A possible evolution scenario of the system was also discussed in the context of the mass vs mass ratio diagram.

• 임산에너지
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• 제21권3호
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• pp.46-53
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• 2002

본 연구에서는 인공피음에 의해서 광조건을 3단계로 달리하여 생육시킨 펜둘라자작나무, 층층나무, 물푸레나무를 대상으로 생장량과 물질생산량 등 특성을 조사하여 생리ㆍ생태적 특성을 밝히고자 연구를 실시하였다. 인공피음처리에 따른 조사 대상 수종의 묘고생장 차이는 거의 없었으며, 근원직경의 생장은 전광처리구가 투광율 7-10%의 피음처리구보다 상대생장율이 29-32% 이상 우수한 생장율을 나타냈다. 하지만 층층나무의 근원직경생장은 투광율 26-34% 처리구에서 높은 생장율을 나타냈다. 대부분의 수종에서 피음처리 수준에 따른 광량감소와 함께 총 물질생산량도 감소하였고, 잎과 줄기의 비율이 뿌리에 비해 증가하는 경향을 보였다. 유묘의 T/R율은 대부분의 수종이 피음의 강도가 강할수록 T/R율이 높아지는 경향으로 전광처리구의 0.51∼l.13보다 투광율 7-10%의 강피음처리구가 1.00∼2.27로 높게 나타냈다. 전체적으로 비교할 때 인공피음처리에 의한 광량이 감소할수록 SLA, LAR, LWR은 광환경의 변화에 따른 피음의 강도가 강할수록 통계적으로 유의적인 차이를 보이며 증가하였다.