Search results for "RARE"

showing 10 items of 2778 documents

OH-related Infrared Absorption Bands in Oxide Glasses

2005

We report the infrared activity, in the spectral region of the OH stretching modes, of different composite silicate glasses whose chemical composition is established by X-ray fluorescence measurements. The analysis of the absorption line profiles is made in terms of different spectral contributions, Gaussian in shape. The comparison with analogous spectra obtained in vitreous silica samples with impurity concentrations < 100 part per million moles is evidence of the effects of the different oxides on the vibrational properties of the OH groups. In particular, for oxide glasses a red shift of the composite band at about 3670 cm(-1), assigned to the OH stretching modes of free Si-OH groups an…

Absorption spectroscopyInfraredFTIR AbsorptionOxide glasseOxideAnalytical chemistryX-ray fluorescenceInfrared spectroscopyCondensed Matter PhysicsCondensed Matter::Disordered Systems and Neural NetworksSylanol groupsSilicateSpectral lineSettore FIS/07 - Fisica Applicata(Beni Culturali Ambientali Biol.e Medicin)Settore FIS/03 - Fisica Della MateriaElectronic Optical and Magnetic Materialschemistry.chemical_compoundchemistryImpurityHydroxyl groupFTIR spectroscopy.Materials ChemistryCeramics and Compositessilicate glasse
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X-shooter spectroscopy of young stars with disks. The TW Hydrae association as a probe of the final stages of disk accretion

2019

We investigate ongoing accretion activity in young stars in the TW Hydrae association (TWA, ~8-10 Myr), an ideal target to probe the final stages of disk accretion down to brown dwarf masses. Our sample comprises eleven TWA members with infrared excess, amounting to 85% of the total TWA population with disks, with spectral types between M0 and M9, and masses between 0.58 and 0.02 Msol. We employed homogeneous spectroscopic data from 300 to 2500 nm, obtained with X-shooter, to derive individual extinction, stellar parameters, and accretion parameters simultaneously. We then examined Balmer lines and forbidden emission lines to probe the physics of the star-disk interaction environment. We de…

AccretionOpen clusters and associations: individual: TWA010504 meteorology & atmospheric sciencesBrown dwarfFOS: Physical sciencesTechniques: spectroscopicAstrophysicsProtoplanetary diskStellar classification01 natural sciencesspectroscopic [Techniques]symbols.namesakeSettore FIS/05 - Astronomia E Astrofisicalow-mass [Stars]pre-main sequence [Stars]0103 physical sciencesStars: low-maTW HydraeQB Astronomy010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QC0105 earth and related environmental sciencesQBEarth and Planetary Astrophysics (astro-ph.EP)PhysicsInfrared excessBalmer seriesAstronomy and AstrophysicsDASAstrophysics - Astrophysics of GalaxiesAccretion (astrophysics)StarsQC PhysicsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAccretion diskAstrophysics of Galaxies (astro-ph.GA)Accretion diskssymbolsStars: pre-main sequenceindividual: TWA [Open clusters and associations]Astrophysics - Earth and Planetary Astrophysics
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TW Hydrae association with X-shooter

2019

Measurements of the protoplanetary disk frequency in young star clusters of different ages indicate disk lifetimes <10Myr. However, our current knowledge of how mass accretion in young stars evolves over the lifespans of disks is subject to many uncertainties, especially at the lower stellar masses. In this study, we investigate ongoing accretion activity in the TW Hydrae association (TWA), the closest association of pre-main sequence stars with active disks. The age (8-10Myr) and the proximity of the TWA render it an ideal target to probe the final stages of disk accretion down to brown dwarf masses. The study is based on homogeneous spectroscopic data from 300nm to 2500nm, obtained synopt…

AccretionUltraviolet astronomyAstrophysics and AstronomyAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstellar astronomyobservational astronomyPre main sequence starsM starsInfrared astronomyAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsPre-main sequence starsAstrophysical ProcessesNatural SciencesAstrophysics::Galaxy AstrophysicsSpectroscopy
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Characterization of particle morphology of biochanin A molecularly imprinted polymers and their properties as a potential sorbent for solid-phase ext…

2014

Abstract Molecularly imprinted polymers (MIPs) with biochanin A as a template were obtained using a bulk polymerization with non-covalent imprinting approach. The polymers were prepared in acetonitrile as porogen, using ethylene glycol dimethacrylate (EDMA) as cross-linking agent. The synthesis, with an application of 1′,1′-azobis(cyclohexanecarbonitrile) (ACHN) as an initiator, has been performed thermally. During the synthesis process the effect of different functional monomers such as methacrylic acid (MAA), acrylamide (AA) and 4-vinylpyridine (4-VP) was investigated. The application of nitrogen sorption porosimetry, scanning electron microscopy (SEM), and Fourier transform infrared spec…

AcetonitrilesMaterials scienceNitrogenPolymersPyridinesEthylene glycol dimethacrylateBioengineeringPolymerizationBiochanin ABiomaterialschemistry.chemical_compoundSpectroscopy Fourier Transform Infraredsolid-phase extractionSolid phase extractionFourier transform infrared spectroscopyChromatography High Pressure Liquidchemistry.chemical_classificationphytoestrogensAcrylamideChromatographySolid Phase ExtractionMolecularly imprinted polymerPolymerGenisteinIsoflavonesCross-Linking ReagentschemistryMethacrylic acidMechanics of MaterialsadsorptionMicroscopy Electron ScanningMethacrylatesmolecular imprintingMolecular imprintingNuclear chemistryMaterials Science & Engineering C-Materials for Biological Applications
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Zur protonenkatalysierten Aralkylierung von 1,2,3-Trimethylindol und 1,2,3,4-Tetrahydrocarbazol mit Arylaldehyden

1987

1,2,3-Trimethylindol (2) liefert mit Benzaldehyden die Kondensationsprodukte 5 und 6, wahrend aus den NH-Indolen 1 und 3 die Verbindungen 7 und 8 entstehen. Proton-catalyzed Aralkylation of 1,2,3-Trimethylindole and 1,2,3,4-Tetrahydrocarbazole with Arylaldehydes Reaction of 1,2,3-trimethylindole (2) with benzaldehydes leads to the condensation compounds 5 and 6, the NH-indoles 1 and 3, however, give 7 and 8.

Acid catalysisBicyclic moleculeChemistryStereochemistryInfraredDrug DiscoveryCondensationPolymer chemistryPharmaceutical ScienceNuclear magnetic resonance spectroscopyArchiv der Pharmazie
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Geochemistry of REE, Zr and HF in a wide range of pH and water composition: The Nevado del Ruiz volcano hydrothermal system (Colombia)

2015

International audience; The geochemical behaviour of Rare Earth Elements, Zr and Hf was investigated in the thermal waters of Nevado del Ruiz volcano system. A wide range of pH, between 1.0 and 8.8, characterizes these fluids. The acidic waters are sulphate dominated with different Cl/SO4 ratios. The important role of the pH and the ionic complexes for the distribution of REE, Zr and Hf in the aqueous phase was evidenced. The pH rules the precipitation of authigenic Fe and Al oxyhydroxides producing changes in REE, Zr, Hf amounts and strong anomalies of Cerium. The precipitation of alunite and jarosite removes LREE from the solution, changing the REE distribution in acidic waters.Y–Ho and Z…

Acidic waterGeochemistrychemistry.chemical_element[SDU.STU]Sciences of the Universe [physics]/Earth SciencesFractionationengineering.materialHydrothermal circulationGeochemistry and PetrologyRare earth elementJarositeIonic complexeZirconiumFe-Al oxyhydroxideAcidic waters; Fe-Al oxyhydroxides; Hafnium; Ionic complexes; Rare earth elements; Zirconium; Geochemistry and Petrology; GeologyGeologyYttriumAuthigenicAlunite6. Clean waterCeriumchemistry13. Climate actionengineeringZirconiumHafniumGeology
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Optical properties of silver halide fibres: ageing effects

1996

The relation between the structure of fibres extruded from mixed silver halides and their IR optical losses and luminescence properties is studied. The recently established ageing effect of the considerable growth of mean grain size of the fibre's polycrystalline structure (typically from 20 to 1000 nm in two years) is correlated with IR and luminescence measurements. IR spectra measured in the interval show growth of the concentrations of molecular impurities. The luminescence measurements are used for the characterization of the fibre's structure ordering. The luminescence decay kinetics is analysed theoretically in terms of the diffusion-controlled recombination of spatially well-correla…

Acoustics and UltrasonicsSilver halideChemistrybusiness.industryAnalytical chemistryInfrared spectroscopyHalideCondensed Matter PhysicsGrain sizeSurfaces Coatings and FilmsElectronic Optical and Magnetic MaterialsGrain growthchemistry.chemical_compoundOpticsImpurityCrystalliteLuminescencebusinessJournal of Physics D: Applied Physics
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Temporal Control of Pulses from a High-Repetition-Rate Tunable Ti:Sapphire Laser by Active Q-switching

2003

We investigated the lasing characteristics of a Ti:sapphire laser pumped by a pulsed high-repetition-rate Nd:YAG laser. The pump laser has a pulsewidth of 450 ns, while the Ti:sapphire laser shows a significantly shorter pulse width of 25 ns for suitably intense pumping. The energy conversion efficiency of the laser is more than 10%. To synchronize different lasers and to avoid multiple spiking during one pump pulse, we use a Brewster-cut Pockels cell in the resonator for Q-switching. The temporal profile and conversion efficiency are determined and compared to theoretical estimates.

Active laser mediumMaterials sciencePhysics and Astronomy (miscellaneous)business.industryFar-infrared laserGeneral EngineeringTi:sapphire laserGeneral Physics and AstronomyLaser pumpingInjection seederLaserQ-switchinglaw.inventionOpticslawLaser power scalingbusinessJapanese Journal of Applied Physics
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Effects of Infrared-A Irradiation on Skin: Discrepancies in Published Data Highlight the Need for an Exact Consideration of Physical and Photobiologi…

2010

Skin exposure to infrared (IR) radiation should be limited in terms of irradiance, exposure time and frequency in order to avoid acute or chronic damage. Recommendations aimed at protecting humans from the risks of skin exposure to IR (e.g. ICNIRP, ACGIH) are only defined in terms of acute effects (e.g. heat pain and cardiovascular collapse), whereas the actual exposure conditions (e.g. spectral distribution, exposure geometry, frequency and number of exposures, thermal exchange with the environment, metabolic energy production and regulatory responses) are not taken into consideration. Since the IR component of solar radiation reaching the Earth's surface is mainly IR-A, and considering th…

Acute effectsMetabolic energyInfrared RaysInfraredChemistrySkin exposureHeat painGeneral MedicineModels TheoreticalRadiationModels BiologicalBiochemistryBiophysical PhenomenaPhotobiologyLawTissue damageHumansIrradiationPhysical and Theoretical ChemistrySkinPhotochemistry and Photobiology
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Analgetische Wirkstoffe, 11. Mitt. Diacylderivate des Butyroguanamins

1986

AcylationChemistryInfraredDrug DiscoveryMass spectrumPharmaceutical ScienceNuclear magnetic resonance spectroscopyMedicinal chemistryArchiv der Pharmazie
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