Search results for "Planetary Science"

showing 10 items of 4367 documents

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 ALHAMBRA survey: 2D analysis of the stellar populations in massive early-type galaxies atz< 0.3

2017

Reproduced with permission from Astronomy & Astrophysics

Stellar populationMetallicityAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicselliptical and lenticular cD [Galaxies]01 natural sciencescDPhotometry (optics)0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsgalaxies: formationgalaxies: elliptical and lenticularSpectroscopy010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics[PHYS]Physics [physics]Physics010308 nuclear & particles physicsphotometry [Galaxies]FísicaAstronomy and Astrophysicsevolution [Galaxies]Astrophysics - Astrophysics of Galaxiesformation [Galaxies]Galaxy2d analysisEarly typeGalaxies: elliptical and lenticular cDgalaxies: photometrySpace and Planetary ScienceSpectral energy distributionAstrophysics::Earth and Planetary Astrophysicsgalaxies: evolution[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
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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 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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Stochastic response of combined primary-secondary structures under seismic input

1992

A technique for non-stationary stochastic analysis of linear combined primary and secondary subsystems subjected to a zero-mean Gaussian base excitation is presented. The proposed technique, based on the use of the Taylor's expansion in evaluating the operators which appear in the step-by-step procedure, does not require the evaluation of the complex eigenproperties of the combined system. Operating in this way, even though the numerical procedure is a conditionally stable one, appears to be more efficient than existing methods to evaluate the dynamic response of such composite systems. It is also shown that the proposed procedure is available whether the seismic input is idealized as a fil…

Stochastic processDifferential equationGaussianAutocorrelationWhite noiseGeotechnical Engineering and Engineering GeologyBase (topology)symbols.namesakeEarth and Planetary Sciences (miscellaneous)Taylor seriessymbolsCalculusAlgorithmMathematics
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Combined dynamic response of primary and multiply connected cascaded secondary subsystems

1991

A method is proposed for the deterministic and stochastic non-stationary analysis of linear composite systems with cascaded secondary subsystems subjected to a seismic input. This method makes it possible to evaluate, by means of a unitary formulation, the deterministic and non-stationary stochastic response of both classically and non-classically damped subsystems and of secondary subsystems multiply supported on the primary one, as well as the ground. The proposed procedure is very efficient from a computational point of view, because of the Kronecker algebra systematically employed. Indeed, by using this algebra, it is possible to obtain in a very compact and elegant form the eigenproper…

Stochastic processFunction (mathematics)Geotechnical Engineering and Engineering GeologyTopologyUnitary stateSecond order momentssymbols.namesakeSimple (abstract algebra)Ordinary differential equationKronecker deltaEarth and Planetary Sciences (miscellaneous)symbolsPoint (geometry)AlgorithmMathematicsEarthquake Engineering & Structural Dynamics
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A paradigm of extreme rainfall pluvial floods in complex urban areas: the flood event of 15 July 2020 in Palermo (Italy)

2021

Abstract. In the last few years, some regions of the Mediterranean area have witnessed a progressive increase in extreme events, such as urban and flash floods, as a response to the increasingly frequent and severe extreme rainfall events, which are often exacerbated by the ever-growing urbanization. In such a context, the urban drainage systems may not be sufficient to convey the rainwater, thus increasing the risk deriving from the occurrence of such events. This study focuses on a particularly intense urban flood that occurred in Palermo (Italy) on 15 July 2020; it represents a typical pluvial flood due to extreme rainfall on a complex urban area that many cities have experienced in rece…

StormwaterContext (language use)Urban areaEnvironmental technology. Sanitary engineeringUrban floodGbest management practicesHuman settlementUrbanizationGeography. Anthropology. RecreationFlash floodGE1-350TD1-1066natural based solutionsQE1-996.5geographygeography.geographical_feature_categoryFlood mythGeologycomplex urban areaEnvironmental sciencesextreme rainfallfloodabilityPluvialGeneral Earth and Planetary Sciencesfloods modelingWater resource managementNatural Hazards and Earth System Sciences
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Pianificazione strategica tra sviluppo locale e policentrismo: alcune evidenze empiriche sul caso siciliano

2009

Strategic planning, local development and policentrism: empirical evidence for Sicily The aim of this paper is the analysis of metropolitan strategic planning in Sicily. Urban areas are becoming important units for territorial cohesion policy and strategic planning represents more and more an important policy instrument. Evidence of a policentric pattern is tested across 30 strategic plans carried out by Sicilian cities in order to derive useful insights for policy implications. Methods and Results This study uses multidimensional scaling and rank-size regressions across Sicilian Functional Urban Areas (FUA) as well as descriptive information drawn from strategic plans in order to identify …

Strategic planningLocal DevelopmentLocale (computer software)Metropolitan arealanguage.human_languagepolicentrismo pianificazione strategica sviluppo localeGeographyOrder (exchange)Regional sciencelanguageGeneral Earth and Planetary SciencesOperations managementMultidimensional scalingEmpirical evidenceSicilianGeneral Environmental Science
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OSL dating of sediments from the Gobi Desert, Southern Mongolia

2010

Abstract The present study focuses on the chronological relationship between alternating dune sand and silty water-lain sediments in the central part of the Khongoryn Els dune field in the Gobi Desert, Southern Mongolia. The 23 m high section evolved from the construction of a natural dam by west–east moving sand dunes and fluvial inundation by a river system from the mountain ranges in the south. To resolve the chronology of events, optically stimulated luminescence (OSL) dating was applied and from sedimentological and geochemical analysis the depositional processes could be characterised. Quartz OSL dating of these sediments is hindered by feldspar contamination. Thus, dating of coarse-g…

StratigraphyFluvialGeologySand dune stabilizationSedimentary depositional environmentPaleontologyGeographieGeologic time scaleEarth and Planetary Sciences (miscellaneous)Aeolian processesChronostratigraphyGeomorphologyHoloceneGeologyChronologyQuaternary Geochronology
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On the thermodynamics of listric faults

2004

We investigate a novel fully coupled thermal-mechanical numerical model of the crust in order to trace the physics of interaction of its brittle and ductile layers. In a unified approach these layers develop in a natural transition as a function of the state variables pressure, deviatoric stress, temperature and strain-rate. We find that the main storage of elastic energy lies in the domain where brittle and ductile strain-rates overlap so that shear zones are attracted to this zone of maximum energy dissipation. This dissipation appears as a local heat source (shear heating). The brittle-ductile transition zone evolves through extreme weakening by thermo-mechanical feedback. The physics of…

Stress (mechanics)BrittlenessCreepShear (geology)Space and Planetary ScienceTransition zoneElastic energyThermodynamicsGeologyDissipationShear zoneGeologyEarth, Planets and Space
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