• Journal of Astronomy and Space Sciences
• /
• v.35 no.1
• /
• pp.1-6
• /
• 2018

The reanalysis of the previously published abundance pattern of mild barium star HD202109 (${\zeta}$ Cyg) and the chemical compositions of 129 thin disk barium stars facilitated the search for possible correlations of different stellar parameters with second ionization potentials of chemical elements. Results show that three valuable correlations exist in the atmospheres of barium stars. The first is the relationship between relative abundances and second ionization potentials. The second is the age dependence of mean correlation coefficients of relative abundances vs. second ionization potentials, and the third one is the changes in correlation coefficients of relative abundances vs. second ionization potentials as a function of stellar spatial velocities and overabundances of s-process elements. These findings demonstrate the possibility of hydrogen and helium accretion from the interstellar medium on the atmospheres of barium stars.

• KIEAE Journal
• /
• v.3 no.3
• /
• pp.51-58
• /
• 2003

This Study aims to evaluate the interior atmospheres of atrium by glass colours. For the purpose, the 1/50 scale model of one-sided atrium was made and images of interior atmospheres were pictured under clear sky conditions. And then, questionnaire surveys were conducted on K university students in department architecture engineering. The survey results were analyzed by SPSS program. Frequency and correlation analysis were performed. As results, clear glass is chosen as the most preferred glass colour in any seasons. And, green and blue glasses are preferred in the order. And then, it is revealed that the main variables affecting satisfaction of interior atmospheres are a little changed by thermal senses of seasons. These variables are "bright", "neat", "warm", "comfort", "stable", "active", "static", "elegant" and "cool" through correlation analysis.

• Journal of Astronomy and Space Sciences
• /
• v.29 no.2
• /
• pp.181-189
• /
• 2012

To broaden the understanding of classical Cepheid structure, evolution and atmospheres, we have extended our continuing secret lives of Cepheids program by obtaining XMM/Chandra X-ray observations, and Hubble space telescope (HST) / cosmic origins spectrograph (COS) FUV-UV spectra of the bright, nearby Cepheids Polaris, ${\delta}$ Cep and ${\beta}$ Dor. Previous studies made with the international ultraviolet explorer (IUE) showed a limited number of UV emission lines in Cepheids. The well-known problem presented by scattered light contamination in IUE spectra for bright stars, along with the excellent sensitivity & resolution combination offered by HST/COS, motivated this study, and the spectra obtained were much more rich and complex than we had ever anticipated. Numerous emission lines, indicating $10^4$ K up to ${\sim}3{\times}10^5$ K plasmas, have been observed, showing Cepheids to have complex, dynamic outer atmospheres that also vary with the photospheric pulsation period. The FUV line emissions peak in the phase range ${\varphi}{\approx}0.8-1.0$ and vary by factors as large as $10{\times}$. A more complete picture of Cepheid outer atmospheres is accomplished when the HST/COS results are combined with X-ray observations that we have obtained of the same stars with XMM-Newton & Chandra. The Cepheids detected to date have X-ray luminosities of log $L_X{\approx}28.5-29.1$ ergs/sec, and plasma temperatures in the $2-8{\times}106$ K range. Given the phase-timing of the enhanced emissions, the most plausible explanation is the formation of a pulsation-induced shocks that excite (and heat) the atmospheric plasmas surrounding the photosphere. A pulsation-driven ${\alpha}^2$ equivalent dynamo mechanism is also a viable and interesting alternative. However, the tight phase-space of enhanced emission (peaking near 0.8-1.0 ${\varphi}$) favor the shock heating mechanism hypothesis.

• Publications of The Korean Astronomical Society
• /
• v.27 no.4
• /
• pp.183-184
• /
• 2012

We present the latest results from the Mission Program NIRLT, the NIR spectroscopic observations of brown dwarfs using the IRC on board AKARI. The near-infrared spectra in the wavelength range between 2.5 and $5.0{\mu}m$ is especially important to study the brown dwarf atmospheres because of the presence of non-blended bands of major molecules, including $CH_4$ at $3.3{\mu}m$, $CO_2$ at $4.2{\mu}m$, CO at $4.6{\mu}m$ and $H_2O$ around $2.7{\mu}m$. Our observations were carried out in the grism-mode resulting in a spectral resolution of ~ 120. In total, 27 sources were observed and 18 good spectra were obtained. We investigate the behavior of three molecular absorption bands, CO, $CH_4$ and $CO_2$, in brown dwarf spectra relative to their spectral types. We find that the $CH_4$ band appears in the spectra of dwarfs later than L5 and CO band is seen in the spectra of all spectral types. $CO_2$ is detected in the spectra of late-L and T type dwarfs.

• Journal of the Korean Society for Heat Treatment
• /
• v.8 no.4
• /
• pp.289-301
• /
• 1995

The effect of Air/$C_3H_8$ gas addition on the compound layer growth of steels nitrocarburised in $NH_3+Air+C_3H_8$ mixed gas atmospheres was investigated. It is considered that amount of residual $NH_3$ was varied according to alternation of Air/$C_3H_8$ mixing ratio and volume content. The compound layer formed from nitrocarburising was composed of ${\varepsilon}-Fe_{2-3}$(C, N) and ${\gamma}^{\prime}-Fe_4$(C, N). According as Air/$C_3H_8$ mixing ratio increased, the superficial content of ${\gamma}^{\prime}-Fe_4$(C, N) within the compound layer was increased, at the same time the growth rate of compound layer and porous layer was increased. In the case of alloy steel at the fixed gas composition, the growth rate of compound layer and porous layer was worse than carbon steel and compound layer phase composition structure primarily consisted of E phase. As the carbon content of materials was increasing in the given gas atmospheres, the growth rate of compound layer and porous layer was increased and the superficial content of ${\varepsilon}-Fe_{2-3}$(C, N) within the compound layer was increased.

• Korean Journal of Metals and Materials
• /
• v.47 no.6
• /
• pp.383-390
• /
• 2009

The effects that processing atmospheres and alloy composition have on the wetting characteristics of Al-Mg alloys on the $SiO_{2}$ substrate were investigated by measuring the wetting angles. It was observed that the wetting behavior of the Al-Mg alloys on the $SiO_{2}$ substrate vary depending on the Mg content of the alloys and atmospheres. The results showed that the contact angle decreases with increasing Mg content, angle is generally larger in the $N_{2}$ atmosphere than in the Ar atmosphere. We discussed the validity of the results obtained from the wetting test on the basis of recent theories and the results observed from the actual penetration tests.

• Korean Journal of Food Science and Technology
• /
• v.32 no.3
• /
• pp.668-673
• /
• 2000

The influence of storage atmosphere on ethylene production, quality attributes and storage injury of 'Tsugaru' apples was investigated. Apples were stored in 1% $O_2+1%\;CO_2,\;1%\;O_2+3%\;CO_2,\;3%\;O_2+1%\;CO_2,\;3%\;O_2+3%\;CO_2$ and air at $0^{\circ}C$ for 5 months. Ethylene production was more suppressed by 1% $O_2$ than 3% $O_2$ atmospheres regardless $CO_2$ levels. The loss of flesh firmness and the decrease of titratable acidity were not significantly different among the storage atmospheres until 3 months of storage but more retarded by 1% $O_2$ than 3% $O_2$ atmospheres thereafter. Soluble solid content was unaffected by the storage atmosphere, but the content tended to be increased until 2 months of storage and then not varied. Ethanol content increased up to a peak level followed by a gradual loss during storage in CA but increased continuously in air. In the sensory evaluation after storage for 5 months, hardness, tartness and overall acceptability of apples stored in 1% $O_2$ atmospheres were significantly higher than those stored in the others. There was no fruit injury or off-flavor production resulting from the 1% $O_2$ atmospheres. The incidence of bitter pit was reduced as storage $O_2$ level decreased. The results show that the optimum conditions of CA storage for 'Tsugaru' apples are $0^{\circ}C$ and 1% $O_2+1{\sim}3%\;CO_2$.

• The Bulletin of The Korean Astronomical Society
• /
• v.25 no.2
• /
• pp.61-61
• /
• 2000

• Bulletin of the Korean Space Science Society
• /
• 2000.10a
• /
• pp.61-61
• /
• 2000

No Abstract, See Full Text

• The Bulletin of The Korean Astronomical Society
• /
• v.7
• /
• pp.9.1-9.1
• /
• 1982