Search results for "velocity"

showing 10 items of 881 documents

The gaia-eso survey: dynamical analysis of the l1688 region in ophiuchus

2016

The Gaia ESO Public Spectroscopic Survey (GES) is providing the astronomical community with high-precision measurements of many stellar parameters including radial velocities (RVs) of stars belonging to several young clusters and star-forming regions. One of the main goals of the young cluster observations is to study of their dynamical evolution and provide insight into their future, revealing if they will eventually disperse to populate the field, rather than evolve into bound open clusters. In this paper we report the analysis of the dynamical state of L1688 in the $\rho$~Ophiuchi molecular cloud using the dataset provided by the GES consortium. We performed the membership selection of t…

Stars: formationPopulationFOS: Physical sciencesAstrophysics01 natural sciencesVirial theoremstars: pre-main sequence / open clusters and associations: individual: L1688 / stars: kinematics and dynamics / stars: formation0103 physical scienceseducation010303 astronomy & astrophysicsQCOpen clusters and associations: individual: L1688Solar and Stellar Astrophysics (astro-ph.SR)QBPhysicseducation.field_of_study010308 nuclear & particles physicsStar formationMolecular cloudVelocity dispersionAstronomy and AstrophysicsStars: kinematics and dynamicAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesStarsAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)OphiuchusStars: pre-main sequenceOpen clusterAstronomy and Astrophysics
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Hot-electron noise suppression in n-Si via the Hall effect

2008

We investigate how hot-electron fluctuations in n-type Si are affected by the presence of an intense (static) magnetic field in a Hall geometry. By using the Monte Carlo method, we find that the known Hall-effect-induced redistribution of electrons among valleys can suppress electron fluctuations with a simultaneous enhancement of the drift velocity. We investigate how hot-electron fluctuations in n-type Si are affected by the presence of an intense (static) magnetic field in a Hall geometry. By using the Monte Carlo method, we find that the known Hall-effect-induced redistribution of electrons among valleys can suppress electron fluctuations with a simultaneous enhancement of the drift vel…

Statistics and ProbabilityCondensed Matter - Materials ScienceQuantum PhysicsDrift velocityNoise suppressionMaterials scienceCondensed matter physicsMonte Carlo methodMaterials Science (cond-mat.mtrl-sci)FOS: Physical sciencesStatistical and Nonlinear PhysicsElectronCondensed Matter::Mesoscopic Systems and Quantum Hall EffectMagnetic fieldhot electrons Si noise Hall effectHall effectRedistribution (chemistry)Statistics Probability and UncertaintyQuantum Physics (quant-ph)Hot electron
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Asymptotics of correlation functions of the Heisenberg-Ising chain in the easy-axis regime

2016

We analyze the long-time large-distance asymptotics of the longitudinal correlation functions of the Heisenberg-Ising chain in the easy-axis regime. We show that in this regime the leading asymptotics of the dynamical two-point functions is entirely determined by the two-spinon contribution to their form factor expansion. Its explicit form is obtained from a saddle-point analysis of the corresponding double integral. It describes the propagation of a wave front with velocity $v_{c_1}$ which is found to be the maximal possible group velocity. Like in wave propagation in dispersive media the wave front is preceded by a precursor running ahead with velocity $v_{c_2}$. As a special case we obta…

Statistics and ProbabilityHigh Energy Physics - Theory[PHYS.COND.GAS]Physics [physics]/Condensed Matter [cond-mat]/Quantum Gases [cond-mat.quant-gas]Correlation functionsWave propagationExact asymptotic resultsGeneral Physics and AstronomyFOS: Physical sciences01 natural sciences010305 fluids & plasmas[ PHYS.COND.GAS ] Physics [physics]/Condensed Matter [cond-mat]/Quantum Gases [cond-mat.quant-gas][ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]Condensed Matter - Strongly Correlated ElectronsQuantum spin chain0103 physical sciencesQuantum communication010306 general physicsDispersion (water waves)Mathematical PhysicsSaddlePhysicsStrongly Correlated Electrons (cond-mat.str-el)[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]Heisenberg modelMultiple integralMathematical analysisForm factor (quantum field theory)Statistical and Nonlinear PhysicsFunction (mathematics)High Energy Physics - Theory (hep-th)Quantum Gases (cond-mat.quant-gas)Modeling and Simulation[ PHYS.COND.CM-SCE ] Physics [physics]/Condensed Matter [cond-mat]/Strongly Correlated Electrons [cond-mat.str-el]Group velocity[PHYS.COND.CM-SCE]Physics [physics]/Condensed Matter [cond-mat]/Strongly Correlated Electrons [cond-mat.str-el]Condensed Matter - Quantum Gases
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High-resolution particle sizing by optical tracking of single colloidal particles

1997

Abstract The motion of individual Brownian particles is observed using the confocal Tracking Microscope recently introduced by Schatzel (K. Schatzel, W. G. Neumann, J. Muller and B. Materzok, App. Opt. 31 (1992) 770–778). Particles are laterally trapped in a strongly focused laser beam. By evaluating the light-pressure-induced drift velocity and the backscattered intensity we are able to detemine particle size histograms with a resolution better than 2%. This is demonstrated on a mixture of seven species of polystyrene latex spheres in the diameter range between 300 and 450 nm, where six classes of diameters are identified. We discuss the scope of the method and potential applications.

Statistics and ProbabilityRange (particle radiation)MicroscopeDrift velocityMaterials sciencebusiness.industryResolution (electron density)Condensed Matter PhysicsTracking (particle physics)law.inventionOpticslawParticleSPHERESParticle sizebusinessPhysica A: Statistical Mechanics and its Applications
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The kinematics of water masers in the stellar molecular outflow source, IRAS 19134+2131

2004

Using the Very Large Array (VLA) and the Very Long Baseline Array (VLBA), we have observed water maser emission in the proto-planetary nebula candidate IRAS 19134+2131, in which the water maser spectrum has two groups of emission features separated in radial velocity by ∼100 km s^−1. The blue-shifted and red-shifted clusters of maser features are clearly separated spatially by ∼150 mas, indicative of a fast collimated flow. However, not all of the maser features are aligned along the axis of the flow, as is seen in the similar high-velocity water maser source, W43A. Comparing the VLA and VLBA maps of the water maser source, we find 4 maser features that were active for 2 years. Using only V…

Stellar kinematicsAstrophysics::High Energy Astrophysical PhenomenaOutflowsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAGB and post-AGBlaw.inventionlawIndividual starsAstrophysics::Solar and Stellar AstrophysicsAsymptotic giant branchOH/IR starMaserMasers stars ; AGB and post-AGB ; Distances ; Kinematics Winds ; Outflows ; Individual stars ; IRAS 19134+2131Astrophysics::Galaxy AstrophysicsVery Long Baseline ArrayPhysicsNebulaKinematics WindsAstronomyIRAS 19134+2131Astronomy and AstrophysicsGalactic plane:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Masers starsDistancesRadial velocitySpace and Planetary ScienceUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Astronomy & Astrophysics
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CGCG 480-022: A Distant Lonesome Merger?

2006

[EN]We present a complete analysis, which includes morphology, kinematics, stellar populations, and N-body simulations, of CGCG 480-022, the most distant (cz = 14,317 km s-1) isolated galaxy studied so far in such detail. The results all support the hypothesis that this galaxy has suffered a major merger event with a companion of ~0.1 times its mass. Morphology reveals the presence of a circumnuclear ring and possibly further ring debris. The radial velocity curve looks symmetrical, while the velocity dispersion increases with radius, reaching values that do not correspond to a virialized system. Moreover, this galaxy deviates significantly from the fundamental plane and the Faber-Jackson r…

Stellar populationFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsKinematicsAstrophysicsabundances [galaxies]kinematics and dynamics [galaxies]galaxies: interactionsgalaxies: kinematics and dynamicsAstrophysics::Galaxy AstrophysicsPhysicsgalaxies: individual (CGCG 480 022)interactions [galaxies]Instituto de Ciencias del PatrimonioStar formationAstrophysics (astro-ph)Velocity dispersionAstronomy and Astrophysicsindividual (CGCG 480 022) [galaxies]GalaxyInstitute of Heritage SciencesRadial velocitySpace and Planetary ScienceIncipitstructure [galaxies]galaxies: structuregalaxies: abundancesAstrophysics::Earth and Planetary AstrophysicsFundamental plane (elliptical galaxies)n-body simulations [methods]methods: n-body simulationsThe Astrophysical Journal
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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 Mean-Field Limit for Solid Particles in a Navier-Stokes Flow

2008

We propose a mathematical derivation of Brinkman's force for a cloud of particles immersed in an incompressible viscous fluid. Specifically, we consider the Stokes or steady Navier-Stokes equations in a bounded domain Omega subset of R-3 for the velocity field u of an incompressible fluid with kinematic viscosity v and density 1. Brinkman's force consists of a source term 6 pi rvj where j is the current density of the particles, and of a friction term 6 pi vpu where rho is the number density of particles. These additional terms in the motion equation for the fluid are obtained from the Stokes or steady Navier-Stokes equations set in Omega minus the disjoint union of N balls of radius epsilo…

Stokes equation01 natural sciencesHomogenization (chemistry)Navier-Stokes equationPhysics::Fluid DynamicsMathematics - Analysis of PDEsFOS: Mathematics[MATH.MATH-AP]Mathematics [math]/Analysis of PDEs [math.AP]Boundary value problem0101 mathematicsMathematical Physics(MSC) 35Q30 35B27 76M50Particle systemPhysicsHomogenization010102 general mathematicsMathematical analysis35Q30 35B27 76M50Stokes equationsStatistical and Nonlinear Physics010101 applied mathematicsFlow velocityDragSuspension FlowsBounded functionCompressibilityBall (bearing)Navier-Stokes equationsAnalysis of PDEs (math.AP)
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1980

A phenomenological theory of the Phase Distribution Chromatography (PDC)-separation effect is outlined and a theoretical equation for the measured PDC-calibration curves is given. Assuming a reversible-thermodynamical equilibrium in the polystyrene-PDC-column, only a relatively small part of the measured PDC-calibration curves could be explained: namely those running below their tangents. In order to explain the whole sigmoidal shape of the experimental curves, a theory of steady state in the system sol/gel was developed assuming deformation of the polymer coil near the gel front due to the stress related to the velocity gradient. The resulting dynamical flow-equilibrium differs highly from…

Stress (mechanics)Partition coefficientPartition function (statistical mechanics)Steady stateChromatographyDeformation (mechanics)ChemistryVelocity gradientPhase (matter)ThermodynamicsTangentDie Makromolekulare Chemie
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Changes in the cerebrovascular effects of endothelin-1 and nicardipine after experimental subarachnoid hemorrhage.

1993

The role of endothelium-related factors in the pathogenesis of cerebral vasospasm after subarachnoid hemorrhage (SAH) has gained interest since the discovery of endothelin-1 (ET-1). We have examined, before and after SAH, the responsiveness of the cerebrovascular bed of the goat to ET-1, the sources of Ca2+ in ET-1-induced responses, and the ability of the Ca2+ entry blocker nicardipine to counteract them. Before SAH, injection of ET-1 into the cerebral circulation increased cerebrovascular resistance, thereby producing dose-dependent reductions in cerebral blood flow (CBF), which were prevented by nicardipine. In isolated middle cerebral arteries, ET-1 induced concentration-dependent contr…

Subarachnoid hemorrhageCerebral arteriesNicardipineBlood PressureCerebral circulationNicardipineCerebral vasospasmHeart RatemedicineAnimalscardiovascular diseasesDose-Response Relationship Drugbusiness.industryEndothelinsGoatsHemodynamicsBrainVasospasmSubarachnoid Hemorrhagemedicine.diseasenervous system diseasesmedicine.anatomical_structureCerebral blood flowVasoconstrictionAnesthesiaSurgeryFemaleVascular ResistanceNeurology (clinical)businessBlood Flow VelocityBlood vesselmedicine.drugNeurosurgery
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