Search results for " clusters"

showing 10 items of 1091 documents

The Gaia-ESO survey: Discovery of a spatially extended low-mass population in the Vela OB2 association

2015

The nearby (distance~350-400 pc), rich Vela OB2 association, includes $\gamma^2$ Velorum, one of the most massive binaries in the solar neighbourhood and an excellent laboratory for investigating the formation and early evolution of young clusters. Recent Gaia-ESO survey observations have led to the discovery of two kinematically distinct populations in the young (10-15 Myr) cluster immediately surrounding $\gamma^2$ Velorum. Here we analyse the results of Gaia-ESO survey observations of NGC 2547, a 35 Myr cluster located two degrees south of $\gamma^2$ Velorum. The radial velocity distribution of lithium-rich pre-main sequence stars shows a secondary population that is kinematically distin…

Stellar populationStars: Individual: Gamma2 velorumPopulationFOS: Physical sciencesTechniques: SpectroscopicAstrophysicsVela01 natural sciencesOpen clusters and associations: Individual: NGC 25470103 physical sciencesCluster (physics)educationStars: Pre-main sequence010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)QBOpen clusters and associations: Individual: Vela OB2Physicseducation.field_of_study010308 nuclear & particles physicsAstronomy and Astrophysicsstars: formation; stars: pre-main sequence; techniques: spectroscopicAstronomy and AstrophysicRadial velocityStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceStars: FormationLow MassOpen clusters and associations: Individual: NGC 2547; Open clusters and associations: Individual: Vela OB2; Stars: Formation; Stars: Individual: Gamma2 velorum; Stars: Pre-main sequence; Techniques: Spectroscopic; Astronomy and Astrophysics; Space and Planetary Science
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The Second APOKASC Catalog: The Empirical Approach

2018

We present a catalog of stellar properties for a large sample of 6676 evolved stars with APOGEE spectroscopic parameters and \textit{Kepler} asteroseismic data analyzed using five independent techniques. Our data includes evolutionary state, surface gravity, mean density, mass, radius, age, and the spectroscopic and asteroseismic measurements used to derive them. We employ a new empirical approach for combining asteroseismic measurements from different methods, calibrating the inferred stellar parameters, and estimating uncertainties. With high statistical significance, we find that asteroseismic parameters inferred from the different pipelines have systematic offsets that are not removed b…

Stellar populationoscillations (including pulsations) [stars]fundamental parameters [stars]KEPLERFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciences0103 physical sciencesOSCILLATIONSAstrophysics::Solar and Stellar AstrophysicsStatistical dispersionstars abundancesFIELD010303 astronomy & astrophysicsRed clumpScalingComputingMilieux_MISCELLANEOUSAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)PhysicsMIXING-LENGTH010308 nuclear & particles physicsAstronomy and AstrophysicsRadiusSurface gravityAGESRED GIANTSStarsStar clusterAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceOPEN CLUSTERSAstrophysics::Earth and Planetary AstrophysicsBOLOMETRIC CORRECTIONS[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]STARSASTEROSEISMIC MASS
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Calculation of modification of alkali metal atomic transition probability in strong external magnetic field and its application

2010

International audience; Interaction of alkali atoms with external magnetic field induced a splitting and a shift of their energy levels. We have study this interaction for external field from 0 to 5000 Gauss when the alkali vapor is confined in submicron thin vapor cell with thickness L = λ/2. Rubidium and Sodium vapors have been studied. The Hamiltonian can be expressed as the sum of the unperturbated atomic Hamiltonian and the so-called Zeeman Hamiltonian. The probability of a transition, induced by the laser electric field is proportional to the square of the transfer coefficients modified by the presence of the magnetic field. We will show that the strong nonlinearity of the transition …

Strong Magnetic FieldTransition Probability[ PHYS.QPHY ] Physics [physics]/Quantum Physics [quant-ph][PHYS.QPHY]Physics [physics]/Quantum Physics [quant-ph]SodiumPhysics::Atomic and Molecular ClustersPhysics::Atomic PhysicsRubidiumNanocells[PHYS.QPHY] Physics [physics]/Quantum Physics [quant-ph]
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Trace determination of 90Sr and 89Sr in environmental samples by collinear resonance ionization spectroscopy

1995

Collinear resonance ionization spectroscopy has been developed as a sensitive technique for fast trace detection of 90Sr and 89Sr in the environment. A detection limit for 90Sr of 107 atoms in the presence of 1017 atoms in the presence of 1017 atoms of stable Strontium has been achieved, while the applicability of the method has been demonstrated on real world samples. After collection and chemical separation, strontium is surface ionized, accelerated to 33keV and mass separated. The ions are neutralized and the emerging fast atoms interact with an argon ion laser beam (γ=364 nm) in a quasi‐collinear geometry. Optical excitation starts from the long‐lived 5s4d3 D2 state of strontium, which …

StrontiumChemistryExcited stateIonizationPhysics::Atomic and Molecular Clusterschemistry.chemical_elementPhysics::Atomic PhysicsAtomic physicsRydberg stateSpectroscopyMass spectrometryCharged particleIonAIP Conference Proceedings
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Crystal structure ofp-toluenesulfonylmethyl isocyanide

2015

The molecule of the commercially available title compound, C9H9NO2S, has crystallographically imposed mirror symmetry, the mirror plane passing through the isocyanide group and thepara-C atoms, the methyl C atom and the S atom of the methyl 4-tolyl sulfone moiety. In the crystal, C—H...O hydrogen-bond interactions link the molecules into chains running parallel to thebaxis.

Sulfonylchemistry.chemical_classificationcrystal structureCrystallographyHydrogen bondMethyl isocyanideIsocyanideGeneral ChemistryCrystal structureisocyanide derivativehydrogen bondingCondensed Matter PhysicsBioinformaticsData ReportsSulfoneCrystalCrystallographychemistry.chemical_compoundchemistryQD901-999Physics::Atomic and Molecular ClustersMoietyGeneral Materials SciencePhysics::Atomic PhysicsPhysics::Chemical PhysicsActa Crystallographica Section E Crystallographic Communications
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The dynamics of magnetic ordering in a natural hemo-ilmenite solid solution

2007

Geophysical Journal International, 169 (3)

Superparamagnetic clustersHemo-ilmeniteMaterials scienceSolid solutionAnalytical chemistryAtmospheric temperature rangeengineering.materialExchange anisotropyEnvironmental magnetism; Exchange anisotropy; Hemo-ilmenite; Low-temperature magnetism; Solid solution; Superparamagnetic clustersCrystallographyMagnetizationEnvironmental magnetismGeophysicsExchange biasGeochemistry and PetrologyFerrimagnetismengineeringAntiferromagnetismLow-temperature magnetismIlmeniteSolid solutionSuperparamagnetismGeophysical Journal International
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Toward a density functional description of liquid pH2.

2010

A finite-temperature density functional approach to describe the properties of parahydrogen in the liquid-vapor coexistence region is presented. The first proposed functional is zero-range, where the density-gradient term is adjusted so as to reproduce the surface tension of the liquid-vapor interface at low temperature. The second functional is finite-range and, while it is fitted to reproduce bulk pH2 properties only, it is shown to yield surface properties in good agreement with experiments. These functionals are used to study the surface thickness of the liquid-vapor interface, the wetting transition of parahydrogen on a planar Rb model surface, and homogeneous cavitation in bulk liquid…

Surface (mathematics)Chemical Physics (physics.chem-ph)Statistical Mechanics (cond-mat.stat-mech)Yield surfaceChemistryThermodynamicsFOS: Physical sciencesFísicaCondensed Matter - Soft Condensed MatterSpin isomers of hydrogenFunctional descriptionSurface tensionPhysics::Fluid DynamicsPlanarWetting transitionPhysics - Chemical PhysicsCavitationPhysics::Atomic and Molecular ClustersSoft Condensed Matter (cond-mat.soft)Physical and Theoretical ChemistryCondensed Matter - Statistical MechanicsThe journal of physical chemistry. A
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Water interaction with perfect and fluorine-doped Co3O4 (100) surface

2015

Abstract We report the results of theoretical investigations of water adsorption on undoped and fluorine-doped Co3O4 (100) surface by means of the plane-wave periodic density functional theory (DFT) calculations combined with the Hubbard-U approach and statistical thermodynamics. We discuss the effect of fluorine-doping of the Co3O4 (100) surface and calculated oxygen evolution reaction overpotential based on the Gibbs free-energy diagram of undoped and F-doped surfaces.

Surface (mathematics)ChemistryDiagramDopingOxygen evolutionchemistry.chemical_elementThermodynamicsGeneral ChemistryOverpotentialCondensed Matter PhysicsPeriodic density functional theoryCondensed Matter::Materials ScienceAdsorptionComputational chemistryCondensed Matter::SuperconductivityPhysics::Atomic and Molecular ClustersFluorineCondensed Matter::Strongly Correlated ElectronsGeneral Materials SciencePhysics::Chemical PhysicsSolid State Ionics
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Quenched molecular dynamics studies on the extraction energy of aluminum atoms

2007

The extraction energy of an aluminum atom is calculated at 0 K as a function of coordination number and defect depth for three surface orientations [(100), (110) and (111)]. For each orientation, atoms are selected and extracted one by one. A linear relationship is obtained between the extraction energy of surface atoms and their coordination numbers (with slight variations due to the geometrical configuration of the atoms). However, the study of the influence of the defect depth on the extraction energy highlights the role played by intrinsic stress on the extraction energy. Copyright © 2008 John Wiley & Sons, Ltd.

Surface (mathematics)Coordination numberchemistry.chemical_element02 engineering and technology01 natural sciencesMolecular physicsStress (mechanics)Molecular dynamicsAluminiumVacancy defect0103 physical sciencesAtomMaterials ChemistryPhysics::Atomic and Molecular Clusters010306 general physicsExtraction (chemistry)Surfaces and InterfacesGeneral Chemistry[CHIM.MATE]Chemical Sciences/Material chemistry021001 nanoscience & nanotechnologyCondensed Matter PhysicsSurfaces Coatings and Filmschemistry[ CHIM.MATE ] Chemical Sciences/Material chemistryAtomic physics0210 nano-technology
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Adsorption of organic compounds at the surface of Enceladus' ice grains. A grand canonical Monte Carlo simulation study

2021

International audience; In this paper, we characterise the adsorption of ethylene, propanol and hexanal molecules on crystalline ice by grand canonical Monte Carlo simulations performed at 236 K, a temperature which is typical of some Enceladus’ environments. We show that at low coverage of the ice surface, the adsorption of propanol and hexanal is driven by the interaction of these molecules with the ice phase and, as a consequence, the adsorbed molecules lie more or less parallel to the ice surface. On the other hand, upon saturation, the adsorbate–adsorbate interactions become more and more important and the molecules tend to become tilted with respect to the surface, the aliphatic chain…

Surface (mathematics)EthyleneMaterials scienceGeneral Chemical EngineeringiceThermodynamics02 engineering and technology01 natural sciencesHexanalPropanolCondensed Matter::Materials Sciencechemistry.chemical_compoundEnceladusAdsorptiontrace gases0103 physical sciencesPhysics::Atomic and Molecular ClustersMoleculeGeneral Materials SciencePhysics::Chemical PhysicsEnceladus[PHYS]Physics [physics]010304 chemical physicsGeneral Chemistry021001 nanoscience & nanotechnologyCondensed Matter PhysicssimulationTrace gasCondensed Matter::Soft Condensed Matterchemistry13. Climate actionadsorption[SDU]Sciences of the Universe [physics]Modeling and SimulationAstrophysics::Earth and Planetary Astrophysics0210 nano-technology[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Information Systems
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