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Ivan L. Andronov,Yonggi Kim,Young-Hee Kim,Joh-Na Yoon,Lidia L. Chinarova,Mariia G. Tkachenko 한국우주과학회 2015 Journal of Astronomy and Space Sciences Vol.32 No.2
We present a by-product of our long term photometric monitoring of cataclysmic variables. 2MASS J18024395 +4003309 = VSX J180243.9 +400331 was discovered in the field of the intermediate polar V1323 Her observed using the Korean 1-m telescope located at Mt. Lemmon, USA. An analysis of the two-color VR CCD observations of this variable covers all the phase intervals for the first time. The light curves show this object can be classified as an Algol-type variable with tidally distorted components, and an asymmetry of the maxima (the O’Connell effect). The periodogram analysis confirms the cycle numbering of Andronov et al. (2012) and for the initial approximation, the ephemeris is used as follows: Min I. BJD = 2456074.4904+0.3348837E . For phenomenological modeling, we used the trigonometric polynomial approximation of statistically optimal degree, and a recent method “NAV” (“New Algol Variable”) using local specific shapes for the eclipse. Methodological aspects and estimates of the physical parameters based on analysis of phenomenological parameters are presented. As results of our phenomenological model, we obtained for the inclination i=90°, M1=0.745M◉, M2=0.854M◉, M=M1+M2=1.599M◉, the orbital separation a=1.65·109m=2.37R◉ and relative radii r1=R1/a=0.314 and r2=R2/a=0.360. These estimates may be used as preliminary starting values for further modeling using extended physical models based on the Wilson & Devinney (1971) code and it's extensions
In-vitro instrumental stimulation of oral breakdown of rice gels with different amylose contents
Yonggi Kim,suyong lee 한국산업식품공학회 2017 학술대회 및 심포지엄 Vol.2017 No.11
In-vitro food mastication has been simulated by incorporating size reduction process, followed by incubation with human saliva. However, they do not suffice to simulate the actual oral breakdown process where disruption by mastication (chewing) and wetting/lubrication by salivation take place simultaneously. In this study, in-vitro oral digestion of rice gels with different amylose contents was simulated by instrumentally performing mastication and salivation. The hardness of artificial saliva-treated rice gels was distinctly lowered with increasing chewing cycles and the rice gels with high amylose contents showed the highest degradation rate. When the rice gels were subjected to non-destructive tomographic analysis, the high amylose rice gels were clearly shown to be favorably fragmented into smaller pieces by chewing, followed by the low and intermediate amylose samples. These results could be explained by their cohesive texture rather than hardness. Therefore, this study may help understanding the changes in the physical properties of cereal-based foods during oral digestion.
Yonggi Kim,Sanhoon Ko,Wanil Cho,Suyong Lee 한국산업식품공학회 2017 학술대회 및 심포지엄 Vol.2017 No.04
Chewing and swallowing disorders such as dysphagia are common in the elderly people whose number is reported to continuously increase throughout the world. With this trend, the aging populations have recently become the global focus of substantial research interest in a variety of industrial fields and the food industry is also no exception. Further studies are also necessary to establish the guidelines or criteria for controlling the food texture for the elderly with different living and cultural backgrounds. An experimental attempt was made to bridge the gap between instrumental and sensory texture in a model solid food system, providing a reference texture range for the elderly diets. For doing so, uniaxial compression was applied to measure the instrumental hardness of corn starch gels that was correlated with their sensory properties perceived by the elderly aged 60 and older. A polynomial trend line was satisfactorily obtained with the formula (y=0.2188x2-5.7917x+38.14) describing the relationship between instrumental hardness and starch concentration. When the instrumental hardness (stress) was correlated with the sensory hardness, a linear correlation was observed with a coefficient of determination (R2=0.879). However, the use of logarithmic transformation exhibited the improved correlation of coefficients. A fairly linear correlation (R2>0.96) was thus observed between the instrumental and sensory hardness by a semi-logarithmic relationship known as Weber-Fechner’s law scale. In principal component analysis, two principal components that accounted for 86.71% of the total variance, separated the gel samples in terms of hardness/springiness and moistness, respectively. The categories of the starch gel samples were subdivided into five groups with different stress ranges. As a result, five categories of food texture could be successfully provided with corresponding stress range and consumer languages that can be used as a reference tool to establish the guideline or criteria for developing the elderly foods.
POORLY STUDIED ECLIPSING BINARIES IN THE FIELD OF DO DRACONIS: V454 DRA AND V455 DRA
Kim, Yonggi,Andronov, Ivan L.,Andrych, Kateryna D.,Yoon, Joh-Na,Han, Kiyoung,Chinarova, Lidia L. The Korean Astronomical Society 2020 Journal of The Korean Astronomical Society Vol.53 No.2
We report an analysis of two poorly studied eclipsing binary stars, GSC 04396-00605 and GSC 04395-00485 (recently named V455 Dra and V454 Dra, respectively). Photometric data of the two stars were obtained using the 1-m Korean telescope of the LOAO operated by KASI while monitoring the cataclysmic variable DO Dra in the frame of the Inter-Longitude Astronomy (ILA) project. We derived periods of 0.434914 and 0.376833 days as well as initial epochs JD 2456480.04281 and JD 2456479.0523, respectively, more accurate than previously published values by factors 9 and 6. The phenomenological characteristics of the mean light curves were determined using the New Algol Variable (NAV) algorithm. The individual times of maxima/minima (ToM) were determined using the newly developed software MAVKA, which outputs accurate parameters using "asymptotic parabola" approximations. The light curves were approximated using phenomenological and physical models. In the NAV algorithm, the phenomenological parameters are well determined. We derived physical parameters using the Wilson-Devinney model. In this model, the best-fit parameters are highly correlated, thus some of them were fixed to reasonable values. For both systems, we find evidence for the presence of a cool spot and estimate its parameters. Both systems can be classified as overcontact binaries of EW type.
X-RAY RADIATIONS OF INTERACTING BINARY 44i BOOTIS
KIM YONGGI,KIM MINSU The Korean Astronomical Society 1996 Journal of The Korean Astronomical Society Vol.29 No.suppl1
In order to study the X-ray radiations from solar type strong interacting binary stars, we have collected X-ray data of 44i Bootis (P=0.2678 days, SP=G2+G2) from the EXOSAT data archive. Preliminarly analysis of a part of these data has been already reported by Vilhu & Heise (1986). In this paper, however, we present a more complete light curve in LE region than the previous work, and some unpublished X-ray light curves and spectrums. Using these new materials a new attempt to find the physical explanation about. some observational characteristic figures in the X-ray light curves and spectrums has been made.