Search results for "Spectroscopic"

showing 10 items of 119 documents

Long-term optical and X-ray variability of the Be/X-ray binary H 1145-619: Discovery of an ongoing retrograde density wave

2017

Multiwavelength monitoring of Be/X-ray binaries is crucial to understand the mechanisms producing their outbursts. H 1145-619 is one of these systems, which has recently displayed X-ray activity. We investigate the correlation between the optical emission and the X-ray activity to predict the occurrence of new X-ray outbursts from the inferred state of the circumstellar disc. We have performed a multiwavelength study of H 1145-619 from 1973 to 2017 and present here a global analysis of its variability over the last 40 years. We have used optical spectra from the SAAO, SMARTS and SALT telescopes and optical photometry from INTEGRAL/OMC and ASAS. We also used X-ray observations from INTEGRAL/…

BrightnessBe starAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectX-ray binarystars: emission-lineFOS: Physical sciencesAstrophysics01 natural sciencesSpectral lineDensity wave theoryPhotometry (optics)X-rays: binariesstars: neutrontechniques: photometric0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysicsmedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsBeAstronomy and AstrophysicsLight curvestars: emission-line BeAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceSkyAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomenatechniques: spectroscopicAstronomy & Astrophysics
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Portable Spectroscopic Techniques for the Non-invasive Identification of two historical yellow pigments: Applications and Practical Challenges

2022

Abstract Decades of technological advances in instrumental analysis have transformed many techniques from laboratory in portable analytical tools with increasing their applicability in situ to the study of cultural heritage. It is known that the painting realisation varies from artist to artist, and the identification of the pigments provides a decisive contribution to trace their authenticity and to support an appropriate restoration work. However, in some cases, due to the complexity of painting composition, it is difficult to distinguish between pigments having a similar chemical composition and colour. Here, a systematic study through combined use of portable non-invasive spectroscopic …

Historyportable spectroscopic techniquesMulti-analytical approachGiallorinoNaples YellowComputer Science ApplicationsEducation
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Coronal properties of active G-type stars in different evolutionary phases

2005

We report on the analysis of XMM-Newton observations of three G-type stars in very different evolutionary phases: the "weak-line" T Tauri star HD 283572, the Zero Age Main Sequence star EK Dra and the Hertzsprung-gap giant star 31 Corn. The X-ray luminosities of the three stars are all in the range 10(30) - 10(31) erg/s. We compare the Emission Measure Distributions of these bright sources, derived from high-resolution X-ray spectra, as well as the pattern of elemental abundances vs. First Ionization Potential (FIP). The results of our analysis suggest that the coronae of these stars are very similar in terms of dominant coronal magnetic structures, in spite of differences in their evolutio…

stars : activitystars : individual : EK DraSettore FIS/05 - Astronomia E AstrofisicaX-rays : starstars : individual : HD 283572stars: individual: 31 Comstars; techniques : spectroscopic; stars : activity; stars : coronae; stars: individual: 31 Com; stars : individual : EK Dra; stars : individual : HD 283572 [X-rays]stars : coronaetechniques : spectroscopic
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Modelling Photoionisation in Isocytosine: Potential Formation of Longer‐Lived Excited State Cations in its Keto Form

2021

Abstract Studying the effects of UV and VUV radiation on non‐canonical DNA/RNA nucleobases allows us to compare how they release excess energy following absorption with respect to their canonical counterparts. This has attracted much research attention in recent years because of its likely influence on the origin of our genetic lexicon in prebiotic times. Here we present a CASSCF and XMS‐CASPT2 theoretical study of the photoionisation of non‐canonical pyrimidine nucleobase isocytosine in both its keto and enol tautomeric forms. We analyse their lowest energy cationic excited states including 2π+ , 2nO+ and 2nN+ and compare these to the corresponding electronic states in cytosine. Investigat…

Models MolecularCASPT2Ultraviolet RaysADNPhysics Atomic Molecular & ChemicalRELAXATION DYNAMICSCASSCFArticleCytosineMOLECULAR WAVE-FUNCTIONSCationsIMPLEMENTATION0307 Theoretical and Computational ChemistryPhysical and Theoretical Chemistry0306 Physical Chemistry (incl. Structural)Radiació ionitzantScience & TechnologyChemical PhysicsMolecular StructureChemistry PhysicalConical IntersectionsPhysicsSPECTROSCOPIC FINGERPRINTSDNAArticlesKetonesPhotochemical ProcessesURACILAtomic and Molecular Physics and OpticsChemistryPhotostability2ND-ORDER PERTURBATION-THEORYPhotoionisationPhysical SciencesANO BASIS-SETSSIMULATION0202 Atomic Molecular Nuclear Particle and Plasma PhysicsCASSCF/CASPT2RNAELECTRON CORRELATIONDNA/RNAChemPhysChem
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Spectroscopic Properties of Nuclear Skyrme Energy Density Functionals

2014

We address the question of how to improve the agreement between theoretical nuclear single-particle energies (SPEs) and experiment. Empirically, in doubly magic nuclei, the SPEs can be deduced from spectroscopic properties of odd nuclei that have one more, or one less neutron or proton. Theoretically, bare SPEs, before being confronted with experiment, must be corrected for the effects of the particle-vibration-coupling (PVC). In the present work, we determine the PVC corrections in a fully self-consistent way. Then, we adjust the SPEs, with PVC corrections included, to empirical data. In this way, the agreement with experiment, on average, improves; nevertheless, large discrepancies still …

PhysicsEmpirical dataNuclear Theoryta114FOS: Physical sciencesGeneral Physics and Astronomyenergy density functionals3. Good healthNuclear Theory (nucl-th)Nuclear physicsnuclear skyrmeEnergy densityNeutronspectroscopic propertiesNuclear theoryPhysical review letters
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The comparison of seven different methods to quantify the amorphous content of spray dried lactose

2006

The purpose of this work was to verify the usefulness, advantages and disadvantages of seven methods that are widely used to detect, and quantify the amorphous contents in pharmaceutical solids. Here, StepScan DSC, a type of modulated temperature calorimetry method, was applied for the first time to quantify amorphicity. The comparison of the analytical methods was undertaken with real (non-artificial) test samples, i.e. spray-dried lactose samples with various degrees of crystallinity. In these samples, it was essential that the amorphous and the crystalline portions are not present as separate particles, which is the case when physical (artificial) mixtures of totally amorphous and totall…

Isothermal microcalorimetryRecrystallization (geology)Chemistryrecrystallizationspectroscopic methodsGeneral Chemical Engineeringx-ray powder diffractionAnalytical chemistryCalorimetrycalorimetric methodsAmorphous solidlactosemoisture sorptionCrystallinityDifferential scanning calorimetryGravimetric analysisamorphicitypharmaceutical compoundsGlass transitionPowder Technology
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High resolution study of the six lowest doubly excited vibrational states of PH2D

2005

Abstract The five lowest doubly excited deformational vibrational bands ν 4  +  ν 6 , 2 ν 6 , ν 3  +  ν 4 , ν 3  +  ν 6 , and 2 ν 3 of PH 2 D have been recorded for the first time using a Bruker 120 HR interferometer with a resolution 0.0033 cm −1 and analysed. Some transitions belonging to a very weak band 2 ν 4 have been also assigned. From the fit 24 and 86, respectively, diagonal and resonance interaction parameters were obtained which reproduce 1089 upper energy levels obtained from more than 4600 assigned transitions with the rms deviation of 0.00059 cm −1 .

[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph]InfraredHigh resolution010402 general chemistry01 natural sciencesNuclear magnetic resonance[PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]0103 physical sciencesVibrational bandsHigh resolutionPhysical and Theoretical ChemistryInfrared spectrumSpectroscopy[PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]Physics010304 chemical physicsResolution (electron density)ResonanceSpectroscopic parametersPH2D moleculeAtomic and Molecular Physics and Optics0104 chemical sciences[ PHYS.PHYS.PHYS-AO-PH ] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph]FTIRExcited stateAtomic physics
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Clerodane diterpenoids from Salvia splendens.

2006

Four new clerodane diterpenoids, salvisplendins A-D (1-4), have been isolated from an acetone extract of the flowers of SalVia splendens, together with an artifact (5), arising from salvisplendin D (4) by addition of diazomethane, and the already known clerodane olearin (6). The structures of the new compounds (1-5) were established mainly by 1D and 2D NMR spectroscopic studies and, in the case of salvisplendin A (1), by chemical correlation with splenolide B (7). Complete 1H and 13C NMR assignments for olearin (6), not published hitherto, are also reported.

StereochemistryPharmaceutical ScienceFlowersSalviaAnalytical ChemistryDiterpenes Clerodanechemistry.chemical_compoundFour new clerodane diterpenoids salvisplendins A-D (1-4) have been isolated from an acetone extract of the flowers of SalVia splendens together with an artifact (5) arising from salvisplendin D (4) by addition of diazomethane and the already known clerodane olearin (6). The structures of the new compounds (1-5) were established mainly by 1D and 2D NMR spectroscopic studies and in the case of salvisplendin A (1) by chemical correlation with splenolide B (7). Complete 1H and 13C NMR assignments for olearin (6) not published hitherto are also reportedDrug DiscoveryOrganic chemistrySalviaNuclear Magnetic Resonance BiomolecularPharmacologychemistry.chemical_classificationPlants MedicinalbiologyMolecular StructureChemistryDiazomethaneOrganic ChemistryCarbon-13 NMRbiology.organism_classificationChemical correlationTerpenoidComplementary and alternative medicineItalyMolecular MedicineDiterpeneTwo-dimensional nuclear magnetic resonance spectroscopyLactoneJournal of natural products
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Identification of Morphological Biosignatures in Martian Analogue Field Specimens Using In Situ Planetary Instrumentation

2008

International audience; We have investigated how morphological biosignatures (i.e., features related to life) might be identified with an array of viable instruments within the framework of robotic planetary surface operations at Mars. This is the first time such an integrated lab-based study has been conducted that incorporates space-qualified instrumentation designed for combined in situ imaging, analysis, and geotechnics ( sampling). Specimens were selected on the basis of feature morphology, scale, and analogy to Mars rocks. Two types of morphological criteria were considered: potential signatures of extinct life ( fossilized microbial filaments) and of extant life (crypto-chasmoendolit…

Meridiani PlanumIn situGeologic Sediments010504 meteorology & atmospheric sciencesMOSSBAUER-SPECTROSCOPYInstrumentationOrigin of LifeAntarctic RegionsMarsGUSEV CRATERExploration of MarsCalcium Sulfate01 natural sciencesCRYPTOENDOLITHIC LICHENSCalcium CarbonateAstrobiologyRAMAN-SPECTROSCOPIC DETECTIONGermanyExobiology0103 physical sciences010303 astronomy & astrophysics0105 earth and related environmental sciencesRemote sensingMartianMineralsPlanetary surfaceSpectrometerMERIDIANI-PLANUMWESTERN-AUSTRALIAMars Exploration ProgramAgricultural and Biological Sciences (miscellaneous)YELLOWSTONE-NATIONAL-PARK13. Climate actionSpace and Planetary ScienceMARS EXPLORATIONAmericasANTARCTIC HABITATSIron CompoundsGeologyHAUGHTON IMPACT STRUCTUREAstrobiology
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Study of a sample of faint Be stars in the exofield of CoRoT

2013

International audience; Context. Be stars are probably the most rapid rotators among stars in the main sequence (MS) and, as such, are excellent candidates to study the incidence of the rotation on the characteristics of their non-radial pulsations, as well as on their internal structure. Pulsations are also thought to be possible mechanisms that help the mass ejection needed to build up the circumstellar disks of Be stars.Aims. The purpose of this paper is to identify a number of faint Be stars observed with the CoRoT satellite and to determine their fundamental parameters, which will enable us to study their pulsation properties as a function of the location in the HR diagram and to searc…

010504 meteorology & atmospheric sciencesBe starHertzsprung–Russell diagramK-type main-sequence starstars: emission-lineAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesSpectral lineBlue stragglersymbols.namesakestars: rotation0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]AstronomyBeAstronomy and Astrophysicsstars: early-typeHerbig Ae/Be starT Tauri starStars[SDU]Sciences of the Universe [physics]Space and Planetary Sciencesymbolsstars: fundamental parametersstars: oscillationsAstrophysics::Earth and Planetary Astrophysicsbinaries: spectroscopicAstronomy & Astrophysics
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