Search results for "Clusters"

showing 10 items of 1274 documents

Reversible isomerization of metal nanoclusters induced by intermolecular interaction

2021

Most inorganic nanoparticles are directly surface-terminated (and -stabilized) by protecting ligands, which could greatly affect the atomic packing and physical/chemical properties of their inorganic cores. Here, we show that the intermolecular interactions between the adsorbed molecules and surface ligands can also affect the core structure of inorganic nanoparticles. Through the coupling/decoupling of cationic surfactants (cetyltrimethylammonium cations, CTA+) and anionic surface ligands (para-mercaptobenzoic acid, p-MBA) in the aqueous phase, we have achieved a reversible transformation between two isomers of [Au25(p-MBA)18]− nanoclusters. The interconversion process between the two isom…

Absorption spectroscopyLigandChemistryGeneral Chemical EngineeringBiochemistry (medical)Intermolecular forceCationic polymerizationGeneral ChemistryPhotochemistryBiochemistryNanoclustersMetalMolecular dynamicsCrystallographyAdsorptionvisual_artMaterials Chemistryvisual_art.visual_art_mediumEnvironmental ChemistryMoleculeDensity functional theoryIsomerizationChem
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UV variability and accretion dynamics in the young open cluster NGC 2264

2015

We explore UV and optical variability signatures for several hundred members of NGC 2264 (3 Myr). We performed simultaneous u- and r-band monitoring over two full weeks with CFHT/MegaCam. About 750 young stars are probed; 40% of them are accreting. Statistically distinct variability properties are observed for accreting and non-accreting cluster members. The accretors exhibit a significantly higher level of variability than the non-accretors, especially in the UV. The amount of u-band variability correlates statistically with UV excess in disk-bearing objects, which suggests that accretion and star-disk interaction are the main sources of variability. Cool magnetic spots, several hundred de…

AccretionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSettore FIS/05 - Astronomia E AstrofisicaStars: low-maAstrophysics::Solar and Stellar Astrophysicsaccretion diskAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Stars: variables: T TauriPhysicsPhotosphereHerbig Ae/BeAstronomy and AstrophysicsAstronomy and AstrophysicUltraviolet: starAccretion (astrophysics)StarsWavelengthAmplitudeAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceOpen clusters and associations: individual: NGC 2264Stars: pre-main sequenceAstrophysics::Earth and Planetary AstrophysicsOpen cluster
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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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Gaia -ESO Survey: Analysis of pre-main sequence stellar spectra

2015

This paper describes the analysis of UVES and GIRAFFE spectra acquired by the Gaia-ESO Public Spectroscopic Survey in the fields of young clusters whose population includes pre-main sequence (PMS) stars. Both methods that have been extensively used in the past and new ones developed in the contest of the Gaia-ESO survey enterprise are available and used. The internal precision of these quantities is estimated by inter-comparing the results obtained by such different methods, while the accuracy is estimated by comparison with independent external data, like effective temperature and surface gravity derived from angular diameter measurements, on a sample of benchmarks stars. Specific strategi…

Accuracy and precisionPopulationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstars: pre-main sequenceSurveysfundamental parameters [Stars]Astronomical spectroscopysurveysAngular diameterpre-main sequence [Stars]Astrophysics::Solar and Stellar AstrophysicsSurveydata analysis [Methods]educationSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsAstronomía y AstrofísicaPhysicseducation.field_of_studygeneral [Open clusters and associations][SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Astronomy and AstrophysicsStars: fundamental parameterAstronomy and AstrophysicEffective temperatureopen clusters and associations: generalSurface gravitymethods: data analysisAccretion (astrophysics)StarsAstrophysics - Solar and Stellar AstrophysicsMethods: data analysis; Open clusters and associations: general; Stars: fundamental parameters; Stars: pre-main sequence; Surveys; Astronomy and Astrophysics; Space and Planetary ScienceSpace and Planetary Science[SDU]Sciences of the Universe [physics]open clusters and associations: general; surveys ; methods: data analysisAstrophysics::Earth and Planetary Astrophysicsstars: fundamental parametersMethods: data analysi
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The history of chemical enrichment in the intracluster medium from cosmological simulations

2017

The distribution of metals in the intracluster medium (ICM) of galaxy clusters provides valuable information on their formation and evolution, on the connection with the cosmic star formation and on the effects of different gas processes. By analyzing a sample of simulated galaxy clusters, we study the chemical enrichment of the ICM, its evolution, and its relation with the physical processes included in the simulation and with the thermal properties of the core. These simulations, consisting of re-simulations of 29 Lagrangian regions performed with an upgraded version of the SPH GADGET-3 code, have been run including two different sets of baryonic physics: one accounts for radiative coolin…

Active galactic nucleusCosmology and Nongalactic Astrophysics (astro-ph.CO)Radiative coolingGalaxies:clusters:general; Galaxies:clusters:Intracluster medium; Methods: numerical; Astronomy and Astrophysics; Space and Planetary ScienceMetallicityFOS: Physical sciencesclusters:Intracluster medium [Galaxies]AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSmoothed-particle hydrodynamicsclusters:general [Galaxies]Intracluster medium0103 physical sciencesGalaxies:clusters:Intracluster medium010303 astronomy & astrophysicsGalaxy clusterAstrophysics::Galaxy AstrophysicsPhysicsnumerical [Methods]Methods: numerical010308 nuclear & particles physicsStar formationAstronomyAstronomy and AstrophysicsAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesGalaxies:clusters:generalSupernova13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics - Cosmology and Nongalactic Astrophysics
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A series expansion of the extended Debye-H�ckel equation and application to linear prediction of stability constants

1996

The Debye-Hückel semiempirical extended equation is frequently used to calculate activity coefficients of chemical species and equilibrium constants at ionic strengths different from those used in their experimental evaluation. A series expansion of the extended Debye-Hückel equation is proposed here and checked with experimental data taken from the literature. The expansion is linear in the ionic parameters and yields a geometrical series which converges rapidly and that enables the accurate calculation of interpolated and extrapolated activity coefficients and equilibrium constants by simple and multiple linear regression without previous knowledge of the ionic parameters.

Activity coefficientSeries (mathematics)ChemistryThermodynamicsLinear predictionAnalytical Chemistrysymbols.namesakeIonic strengthComputational chemistryDebye–Hückel equationLinear regressionPhysics::Atomic and Molecular ClusterssymbolsSeries expansionEquilibrium constantTalanta
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Adenosine monophosphate-capped gold(i) nanoclusters: synthesis and lanthanide ion-induced enhancement of their luminescence

2016

Reduction of Au3+ in the presence of just adenosine 5′-monophosphate (AMP) and a zwitterionic organic chemical buffering agent, specifically 4-(2-hydroxyethyl)-1-piperazineethanesulfonic acid (HEPES), combined with light exposure, gives rise to luminescent, water-soluble Au+ nanoclusters (Au+ NCs). The photoluminescence of these NCs is considerably enhanced by adding Y3+ or the chemically similar Yb3+ lanthanide that leads to Au+/Y3+ and Au+/Yb3+ NCs, respectively. These NCs are characterised by absorption (steady-state), photoluminescence (steady-state and time-resolved), and X-ray photoelectron spectroscopy.

Adenosine monophosphateHEPESLanthanidePhotoluminescenceGeneral Chemical Engineering02 engineering and technologyGeneral Chemistry010402 general chemistry021001 nanoscience & nanotechnologyPhotochemistry01 natural sciences0104 chemical sciencesNanoclusterschemistry.chemical_compoundchemistryX-ray photoelectron spectroscopyAbsorption (chemistry)0210 nano-technologyLuminescenceRSC Advances
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Sporting habits of urban runners: Classification according to their motivation

2019

This study analyses the sporting habits of runners participating in short-distance urban running events to identify groups with different motivations towards the practice of endurance running and participation in urban running events. A sample consisting of 937 participants in the Valencia running circuit was interviewed using a questionnaire consisting of a scale of 22 items to analyse their motives for participating in popular races. An exploratory and confirmatory factorial analysis was carried out to check the validity of the instrument, and the analysis identified the following four factors into which the indicators were grouped: psychological and physical motives (3 items), social mot…

AdultMaleTypologyUrban PopulationHealth Toxicology and MutagenesisApplied psychologySample (statistics)ArticleRunningHabits03 medical and health sciences0302 clinical medicinemotivesurban runnersSurveys and Questionnairescitizens’ sports habitsHumans0501 psychology and cognitive sciences030212 general & internal medicineclustersrunnersEsportsMotivation05 social sciencesPublic Health Environmental and Occupational HealthMiddle AgedSocial recognition050106 general psychology & cognitive sciencesAnnual incomeCorredors (Esports)Scale (social sciences)FemaleFactorial analysistypologysportsPsychology
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Amateur Runners’ Commitment: An Analysis of Sociodemographic and Sports Habit Profiles

2020

The aim of this work is to analyse the commitment to running among urban runners by identifying groups regarding commitment to this sport and by defining their sociodemographic profile and their sports habits. A sample of 1806 participants in popular urban races in the city of Valencia was interviewed using an 11-item questionnaire on commitment to running, sociodemographic characteristics, and sports habits. The psychometric properties of the running-commitment scale allowed for the identification of two factors in commitment to running: enthusiasm for running (6 items) and affliction from running (5 items). Subsequently, a cluster analysis combining hierarchical and non-hierarchical metho…

AdultMaleamateur runnersHealth Toxicology and Mutagenesismedia_common.quotation_subjectrunning addictionlcsh:Medicine050109 social psychologysports habitsArticleRunningHabits0504 sociologyurban runnersSurveys and QuestionnairesHumans0501 psychology and cognitive sciencesclustersrunnersmedia_commonEnthusiasmcommitment to runningAddiction05 social scienceslcsh:RPublic Health Environmental and Occupational Health050401 social sciences methodsMiddle AgedBehavior AddictiveAthletesScale (social sciences)FemaleHabitPsychologyAmateurAttitude to HealthDemographyInternational Journal of Environmental Research and Public Health
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Longitudinal Study on Sustained Attention to Response Task (SART): Clustering Approach for Mobility and Cognitive Decline

2022

The Sustained Attention to Response Task (SART) is a computer-based go/no-go task to measure neurocognitive function in older adults. However, simplified average features of this complex dataset lead to loss of primary information and fail to express associations between test performance and clinically meaningful outcomes. Here, we combine a novel method to visualise individual trial (raw) information obtained from the SART test in a large population-based study of ageing in Ireland and an automatic clustering technique. We employed a thresholding method, based on the individual trial number of mistakes, to identify poorer SART performances and a fuzzy clusters algorithm to partition the da…

AgingHealth (social science)SART cognition fuzzy clusters mobility decline multimodal visualization repeated measures specificity sustained attention to response task thresholdsustained attention to response task; SART; multimodal visualization; threshold; fuzzy clusters; cognition; repeated measures; mobility decline; specificityGeriatrics and GerontologySettore MAT/07 - Fisica MatematicaGerontologyGeriatrics
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