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Kovalev, Valeri V,Khotimchenko, Maxim Y,Khotimchenko, Yuri S Kyung Hee Oriental Medicine Research Center 2007 Oriental pharmacy and experimental medicine Vol.7 No.2
Metal binding activity of the pectin samples with different physicochemical properties was studied. It was found that in vitro copper binding capacity of pectins is depending on the following factors: degree of esterification, content of non-methylated anhydrogalacturonic acid, and pH of solution. There was found that the maximum copper uptake capacity increases correspondingly to reduction of the degree of esterification of pectin, rise of the non-methylated anhydrogalacturnic acid content and the solution pH. It is proposed to use for standardization of pectin samples such parameters as the degree of esterification, content of anhydrogalacturonic acid, and intrinsic viscosity.
Yuri S Khotimchenko,Valeri V Kovalev,Maxim Y Khotimchenko 경희대학교 융합한의과학연구소 2007 Oriental Pharmacy and Experimental Medicine Vol.7 No.2
Metal binding activity of the pectin samples with different physicochemical properties was studied. It was found that in vitro copper binding capacity of pectins is depending on the following factors: degree of esterification, content of non-methylated anhydrogalacturonic acid, and pH of solution. There was found that the maximum copper uptake capacity increases correspondingly to reduction of the degree of esterification of pectin, rise of the non-methylated anhydrogalacturnic acid content and the solution pH. It is proposed to use for standardization of pectin samples such parameters as the degree of esterification, content of anhydrogalacturonic acid, and intrinsic viscosity.
Khotimchenko, Yuri S.,Kolenchenko, Elena A.,Khotimchenko, Maxim Y.,Kovalev, Valeri V. Kyung Hee Oriental Medicine Research Center 2004 Oriental pharmacy and experimental medicine Vol.4 No.1
The purpose of this study was to investigate the pharmacological effects of low-esterified pectin on carbon tetrachloride $(CCL_4)-induced$ hepatotoxicity in rats. The study included two experiments. In the first experiment the animals were given daily $CCL_4$ through gavage for 7 days and then 10, 50, or 250 mg/kg b.w. of pectin for 21 days. At the end of experiment rats were killed within 24 hours. The increased bilirubin level, enhanced alanine aminotransferase and aspartate aminotransferase activity in plasma induced by $CCL_4$ were partly normalized by pectin administration in a dose-dependent manner. The pectin treatment also resulted in significant recovery of $CCL_4-induced$ decrease of the liver glycogen content. In addition, pectin significantly improved $CCL_4-induced$ alterations of pro-oxidant and antioxidant biochemical parameters in liver and plasma compared to those of rats administered $CCL_4$. In the second experiment the animals were given daily 10, 50 or 250 mg/ kg b.w. of pectin for 21 days before a 7-day administration of $CCL_4$. Rats were killed 24 hours after the end of experiment. Pretreatment with pectin before $CCL_4$ administration resulted in significantly inhibited increase of the blood enzymatic activities of alanine and aspartate aminotransferases and bilirubin level in a dose-dependent manner. Also, preliminary administration of pectin prevented elevation of malondialdehyde and conjugated diene levels in liver and plasma as well as a reduction of glutathione content in liver of rats given $CCL_4$. These results suggest that low-esterified pectin exert healing and preventive effects on $CCL_4-induced$ hepatotoxicity in rats.
The Scattering and Intrinsic Structure of Sagittarius A* at Radio Wavelengths
Johnson, Michael D.,Narayan, Ramesh,Psaltis, Dimitrios,Blackburn, Lindy,Kovalev, Yuri Y.,Gwinn, Carl R.,Zhao, Guang-Yao,Bower, Geoffrey C.,Moran, James M.,Kino, Motoki,Kramer, Michael,Akiyama, Kazunor American Astronomical Society 2018 The Astrophysical journal Vol.865 No.2
Global millimeter VLBI array survey of ultracompact extragalactic radio sources at 86 GHz
Nair, Dhanya G.,Lobanov, Andrei P.,Krichbaum, Thomas P.,Ros, Eduardo,Zensus, Johann Anton,Kovalev, Yuri Y.,Lee, Sang-Sung,Mertens, Florent,Hagiwara, Yoshiaki,Bremer, Michael,Lindqvist, Michael,de Vice Springer-Verlag 2019 Astronomy and astrophysics Vol.622 No.-
<P><I>Context</I>. Very long baseline interferometry (VLBI) observations at 86 GHz (wavelength, <I>λ</I> = 3 mm) reach a resolution of about 50 <I>μ</I>as, probing the collimation and acceleration regions of relativistic outflows in active galactic nuclei (AGN). The physical conditions in these regions can be studied by performing 86 GHz VLBI surveys of representative samples of compact extragalactic radio sources.</P><P><I>Aims</I>. To extend the statistical studies of compact extragalactic jets, a large global 86 GHz VLBI survey of 162 compact radio sources was conducted in 2010-2011 using the Global Millimeter VLBI Array (GMVA).</P><P><I>Methods</I>. The survey observations were made in a snapshot mode, with up to five scans per target spread over a range of hour angles in order to optimize the visibility coverage. The survey data attained a typical baseline sensitivity of 0.1 Jy and a typical image sensitivity of 5 mJy beam<SUP>−1</SUP>, providing successful detections and images for all of the survey targets. For 138 objects, the survey provides the first ever VLBI images made at 86 GHz. Gaussian model fitting of the visibility data was applied to represent the structure of the observed sources and to estimate the flux densities and sizes of distinct emitting regions (components) in their jets. These estimates were used for calculating the brightness temperature (<I>T</I>b) at the jet base (core) and in one or more moving regions (jet components) downstream from the core. These model-fit-based estimates of <I>T</I>b were compared to the estimates of brightness temperature limits made directly from the visibility data, demonstrating a good agreement between the two methods.</P><P><I>Results</I>. The apparent brightness temperature estimates for the jet cores in our sample range from 2.5 × 10<SUP>9</SUP> K to 1.3 × 10<SUP>12</SUP> K, with the mean value of 1.8 × 10<SUP>11</SUP> K. The apparent brightness temperature estimates for the inner jet components in our sample range from 7.0 × 10<SUP>7</SUP> K to 4.0 × 10<SUP>11</SUP> K. A simple population model with a single intrinsic value of brightness temperature, <I>T</I>0, is applied to reproduce the observed distribution. It yields <I>T</I>0 = (3.77−0.14<SUP>+0.10</SUP>) × 10<SUP>11</SUP> K for the jet cores, implying that the inverse Compton losses dominate the emission. In the nearest jet components, <I>T</I>0 = (1.42−0.19<SUP>+0.16</SUP>) × 10<SUP>11</SUP> K is found, which is slightly higher than the equipartition limit of ∼5 × 10<SUP>10</SUP> K expected for these jet regions. For objects with sufficient structural detail detected, the adiabatic energy losses are shown to dominate the observed changes of brightness temperature along the jet.</P>