• Title/Summary/Keyword: Mass spectroscopy

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Phytochemical Compounds from the Ethanolic Extract of Gymnema sylvestre, Senna auriculata and Cissus quadrangularis through GC-MS Analysis

  • Sindhuja G;Mary Agnes A
    • Mass Spectrometry Letters
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    • v.14 no.2
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    • pp.25-35
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    • 2023
  • Plants are a traditional source of many chemicals used as biochemical, flavors, food, color, and pharmaceuticals in various countries, especially India. Most herbal medicines and their derivatives are often made from crude extracts containing a complex mixture of various phytochemical chemical components (secondary metabolites of the plants). This study aimed to identify bioactive compounds from the different parts of the plant from the ethanolic extract of Gymnema sylvestre, Senna auriculata, and Cissus quadrangularis (leaves, flower, stem) by gas chromatography-mass spectroscopy (GC-MS). The gas chromatography - mass spectrometry analysis revealed the presence of various compounds like 3,4-dimethylcyclohexanol, hexanoic acid, D-mannose, and N-decanoic acid. Hence, the Gymnema sylvestre, Senna auriculata, and Cissus quadrangularis may have chemopreventive, anti-cancer, anti-microbial activity, antioxidant, anti-diabetic activity, anti-inflammatory, and antifungal due to the presence of secondary metabolites in the ethanolic extract. These phytochemicals are supported for traditional use in a variety of diseases.

Characteristics of the NO/$N_2O$ Nitrided Oxide and Reoxidized Nitrided Oxide for NVSM (비휘발성 기억소자를 위한 NO/$N_2O$ 질화산화막과 재산화 질화산화막의 특성에 관한 연구)

  • 이상은;서춘원;서광열
    • Journal of the Korean Vacuum Society
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    • v.10 no.3
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    • pp.328-334
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    • 2001
  • The characteristics of $NO/N_2O$ nitrided oxide and reoxidized nitrided oxide being studied as super thin gate oxide and gate dielectric layers of nonvolatile semiconductor memory(NVSM) was investigated by dynamic secondary ion mass spectrometry(D-SMS), time-of-flight secondary ion mass spectrometry(ToF-SIMS), and x-ray photoelectron spectroscopy (XPS). The specimen was annealed in $NO/N_2O$ ambient after initial oxide process. The result of D-SIMS exhibits that the center of nitrogen exists at the initial oxide interface and the distribution of nitrogen is wider in the annealing process with $N_2O$ than with NO annealing process. For investigating the condition of nitrogen that exists within the nitrided oxide, ToF-SIMS and XPS analysis were carried out. It was shown that the center of nitrogen investigated by D-SIMS was expected the SiON chemical bonds. The nitrogen near the newly formed reoxide/silicon substrate interface was appeared as $Si_2NO$ chemical bonds, and it is agreed with the distribution of SiN and $Si_2NO$ species by ToF-SIMS.

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SMBH Mass Estimate Discrepancy and Its Origin of NGC 6861

  • Jang, Minsung;Owers, Matt
    • The Bulletin of The Korean Astronomical Society
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    • v.37 no.2
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    • pp.69.2-69.2
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    • 2012
  • NGC 6861 is the brightest S0 galaxy in the Telescopium group. It has unusually high central stellar velocity dispersion (~400 km/s) and clear rotation (~250 km/s). Considering the well-known M-sigma relation, this large central dispersion implies that the central supermassive black hole (SMBH) has mass comparable to the most massive black holes in the Universe. However, the mass implied by the bulge luminosity-SMBH mass relation is an order of magnitude lower than that predicted by the M-sigma relation. In order to determine the origin of this inconsistency, we obtain integral field spectroscopy using the Wide Field Spectrograph (WiFeS) on the ANU 2.3m telescope. The data are used to map the velocity and velocity dispersion fields which show that our measurements are consistent with those from the other literature. The large field of view the WiFeS observations have allows us to map the kinematics of a much greater portion of NGC 6861 and reveals that the eastern part of the galaxy has higher velocity and dispersion than the rest of halo. We discuss the origin of the unusual fast rotation and the discrepancy of two SMBH mass estimations from three plausible perspectives: 1) the interaction between subgroups of NGC 6861 and its counterpart, NGC 6868; 2) the inhibited growth of the stellar bulge by the AGN activity which leads to an underestimate the SMBH mass when using the bulge luminosity-SMBH mass relation; and 3) gas rich minor mergers that could be crucial for increasing both rotation velocity and velocity dispersion during the evolution of NGC 6861.

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Inclusion Complex of $Permethylated-{\bata}-Cyclodextrin$ with Benzaldehyde

  • Choi Hee-Sook
    • Bulletin of the Korean Chemical Society
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    • v.13 no.2
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    • pp.179-183
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    • 1992
  • A stable solid new inclusion complex with benzaldehyde and $permethyl-\beta-cyclodextrin$ was obtained by recrystallization method. The structure of the $benzaldehyde-permethyl-\beta-cyclodextrin$ inclusion complex in the solid and solution state have been studied by UV, IR, $^1H-NMR$, $^{13}C-NMR$ and FAB-mass spectroscopy.

Effect of Organic Solvent Extractives on Korean Softwoods Classification Using Near-infrared Spectroscopy

  • Yeon, Seungheon;Park, Se-Yeong;Kim, Jong-Hwa;Kim, Jong-Chan;Yang, Sang-Yun;Yeo, Hwanmyeong;Kwon, Ohkyung;Choi, In-Gyu
    • Journal of the Korean Wood Science and Technology
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    • v.47 no.4
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    • pp.509-518
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    • 2019
  • This study analyzed the effect of organic solvent extractives on the classification of wood species via near-infrared spectroscopy (NIR). In our previous research, five species of Korean softwood were classified into three groups (i.e., Cryptomeria japonica (cedar)/Chamaecyparis obtuse (cypress), Pinus densiflora (red pine)/Pinus koraiensis (Korean pine), and Larix kaempferi (Larch)) using an NIR-based principal component analysis method. Similar tendencies of extractive distribution were observed among the three groups in that study. Therefore, in this study, we qualitatively analyzed extractives extracted by an organic solvent and analyzed the NIR spectra in terms of the extractives' chemical structure and band assignment to determine their effect in more detail. Cedar/cypress showed a similar NIR spectra patterns by removing the extractives at 1695, 1724, and 2291 nm. D-pinitol, which was detected in cedar, contributed to that wavelength. Red pine/Korean pine showed spectra changes at 1616, 1695, 1681, 1705, 1724, 1731, 1765, 1780, and 2300 nm. Diterpenoids and fatty acid, which have a carboxylic group and an aliphatic double bond, contributed to that wavelength. Larch showed a catechin peak in gas chromatography and mass spectroscopy analysis, but it exhibited very small NIR spectra changes. The aromatic bond in larch seemed to have low sensitivity because of the 1st overtone of the O-H bond of the sawdust cellulose. The three groups sorted via NIR spectroscopy in the previous research showed quite different compositions of extractives, in accordance with the NIR band assignment. Thus, organic solvent extractives are expected to affect the classification of wood species using NIR spectroscopy.

3-D Atom Probe Tomography and Secondary ion Mass Spectroscopy techniques for the microstructure and atomic scale investigation on the state of Boron in Steels (3차원 원자 침 분석기 (3-DAPT)와 이차이온 질량분석기 (SIMS)을 이용한 보론 첨가 강의 미세구조와 보론의 원자 단위 분석)

  • Seol, J.B.;Kang, J.S.;Yang, Y.S.;Park, C.G.
    • Proceedings of the Korean Society for Technology of Plasticity Conference
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    • 2008.10a
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    • pp.91-94
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    • 2008
  • Newly developed Atom Probe Tomography (APT) technique can provide the highest available spatial resolution, 3D tomography imaging and quantitative chemical analysis in a sub-nm scale. As a complementary technique to APT, Nano-secondary ion Mass Spectroscopy (SIMS) also provides the boron distribution in micro-scale. Therefore, the exact behavior of boron at either grain boundary or grain interior in steels can be investigated by the combination of APT and SIMS techniques from the sub-nanometer scale to the micrometer scale. The results obtained by both APT and SIMS revealed that the boron atoms were mainly segregated to the grain boundaries rather than to the grain interior in the steels containing 50ppm and 100ppm boron. It also found that carbon atoms were segregated at the boron enriched regions, which were thought to be retained austenite phase due to the chemical composition of carbon atoms.

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New Family of Monoglucosylglyceride Diacyl Glycerol Lipids Containing Very Long Chain bifunctional Acyl Chains in Sarcina ventriculi

  • Jung, Seun-Ho;Chi, Yong-Hoon;Chang, Yoon-Seok;Yi, Dong-Heui;Kwon, Tae-Jong;Hollingsworth, Rawle I.
    • Journal of Microbiology and Biotechnology
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    • v.10 no.3
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    • pp.386-393
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    • 2000
  • Recent research on the fatty acyl chains in the membrane lipids in Sarcina ventriculi has shown that unusually long chain bifunctional fatty acyl components are the major components of the total lipid. However, these studies did not yield any information on the complete structures of the lipid species containing these fatty acids. In this study, the structures of a new family of glucolipids containing bifunctional acyl chains are described. These structures were determined using NMR(Nuclear Magnetic Resonance) Spectroscopy, GC (Gas Chromatography)/MS (Mass Spectrometry), FTIR (Fourier Transform Infrared) spectroscopy, and FAB (Fast Atom Bombardment) mass spectrometric studies. One of the major bifunctional acyl components of the $\alpha$-glucolipids was an $\omega$-formylmethyl ester indicating the presence of plasmalogen. The general structure of the lipid components was one in which the two head groups were separated by a membrane-spanning acyl species. One head group component is a glycerol moiety of each head group, and the other is a glyceryl clucoside. Two regular chain fatty acids, one on the glycerol moiety of each head group, are also present and meet in the middle of the membrane, roughly equidistant from each head group.

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Warm Dust and Gas of Massive YSOs Revealed by Herschel PACS Spectroscopy

  • Kwon, Woojin;van der Tak, Floris F.S.;Karska, Agata;Herczeg, Gregory J.;Chavarria, Luis;Herpin, Fabrice;Wyrowski, Friedrich;Braine, Jonathan;van Dishoeck, Ewine F.
    • The Bulletin of The Korean Astronomical Society
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    • v.40 no.2
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    • pp.41.3-41.3
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    • 2015
  • As part of the Herschel key program "Water in Star-forming Regions with Herschel (WISH)", PACS imaging spectroscopy data have been taken toward ten massive young stellar objects (YSOs): four high mass protostellar objects (HMPOs), two hot molecular cores (HMCs), and four ultracompact HII regions (UCHIIs). The spectra cover a broad range of wavelengths (55 to 210 micron) presenting various atomic and molecular lines as well as excellent dust thermal continua. By fitting the continua utilizing a modified black-body formula we estimate mass-weighted temperature and column density distributions of warm dust and find that UCHII regions are warmer and HMCs are more deeply embedded than the other types. We also estimate rotational temperature and column density distributions of warm CO gas using the rotational diagram analysis. In addition, based on the comparison of high J CO line fluxes to the RATRAN estimates of central heating envelope models, we find that majority of warm CO is originated from bipolar outflow shocks.

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