Search results for "Planetary Science"

showing 10 items of 4367 documents

MILES extended: Stellar population synthesis models from the optical to the infrared

2016

We present the first single-burst stellar population models which covers the optical and the infrared wavelength range between 3500 and 50000 Angstrom and which are exclusively based on empirical stellar spectra. To obtain these joint models, we combined the extended MILES models in the optical with our new infrared models that are based on the IRTF (Infrared Telescope Facility) library. The latter are available only for a limited range in terms of both age and metallicity. Our combined single-burst stellar population models were calculated for ages larger than 1 Gyr, for metallicities between [Fe/H] = -0.40 and 0.26, for initial mass functions of various types and slopes, and on the basis …

CAII TRIPLETStellar populationInfraredMetallicityINITIAL MASS FUNCTIONBROWN DWARFSInfrared telescopeFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstronomical spectroscopyinfrared: galaxiesATMOSPHERIC PARAMETERS0103 physical sciencesRange (statistics)Astrophysics::Solar and Stellar Astrophysics2.5 MU-MGIANT BRANCH STARS010303 astronomy & astrophysicsinfrared: starsEMPIRICAL CALIBRATIONAstrophysics::Galaxy AstrophysicsPhysics010308 nuclear & particles physicsNear-infrared spectroscopyHIGH-SPECTRAL-RESOLUTIONAstronomy and AstrophysicsEVOLUTIONARY SYNTHESISAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)NEWTON-TELESCOPE LIBRARYgalaxies: stellar contentAstrophysics::Earth and Planetary Astrophysics
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ALMA spectral survey of Supernova 1987A – molecular inventory, chemistry, dynamics and explosive nucleosynthesis

2017

We report the first molecular line survey of Supernova 1987A in the millimetre wavelength range. In the ALMA 210--300 and 340--360 GHz spectra, we detected cold (20--170 K) CO, 28SiO, HCO+ and SO, with weaker lines of 29SiO from ejecta. This is the first identification of HCO+ and SO in a young supernova remnant. We find a dip in the J=6--5 and 5--4 SiO line profiles, suggesting that the ejecta morphology is likely elongated. The difference of the CO and SiO line profiles is consistent with hydrodynamic simulations, which show that Rayleigh-Taylor instabilities cause mixing of gas, with heavier elements much more disturbed, making more elongated structure. We obtained isotopologue ratios of…

CIRCUMSTELLAR RINGMetallicityLINE EMISSIONINFRARED WATER-VAPORFOS: Physical sciencesAstrophysics01 natural sciences7. Clean energySpectral lineISM [radio lines]CORE-COLLAPSE SUPERNOVAENucleosynthesis0103 physical sciencesIsotopologueEjectaSupernova remnantLarge Magellanic CloudCARBON-MONOXIDE010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)molecules [ISM]QBHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsabundances [ISM]010308 nuclear & particles physicssupernova remnants [ISM]II-P SUPERNOVAEAstronomyindividual: Supernova 1987A [supernovae]NEBULA M 1-92Astronomy and AstrophysicsSupernovaAstrophysics - Solar and Stellar AstrophysicsPhysics and Astronomy13. Climate actionSpace and Planetary ScienceLARGE-MAGELLANIC-CLOUDAstrophysics - High Energy Astrophysical PhenomenaMASSIVE STARSSN 1987AMonthly Notices of the Royal Astronomical Society
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Degassing at the Volcanic/Geothermal System of Kos (Greece): Geochemical Characterization of the Released Gases and CO2 Output Estimation

2019

Forty-five gas samples have been collected from natural gas manifestations at the island of Kos—the majority of which are found underwater along the southern coast of the island. On land, two anomalous degassing areas have been recognized. These areas are mainly characterized by the lack of vegetation and after long dry periods by the presence of sulfate salt efflorescence. Carbon dioxide is the prevailing gas species (ranging from 88 to 99%), while minor amounts of N2 (up to 7.5%) and CH4 (up to 2.1%) are also present. Significant contents of H2 (up to 0.2%) and H2S (up to 0.3%) are found in the on-land manifestations. Only one of the underwater manifestations is generally rich in N2 (up t…

CO2 outputgeographygeography.geographical_feature_categoryGreece010504 meteorology & atmospheric sciencesArticle Subjectlcsh:QE1-996.5Geochemistry010502 geochemistry & geophysics01 natural sciencesSettore GEO/08 - Geochimica E VulcanologiaCharacterization (materials science)lcsh:Geologyvolcanic arcVolcanoAegean SeaGeneral Earth and Planetary SciencesVolcanic degassingGeothermal gradientGeology0105 earth and related environmental sciencesGeofluids
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CODEX Weak Lensing Mass Catalogue and implications on the mass-richness relation

2021

The COnstrain Dark Energy with X-ray clusters (CODEX) sample contains the largest flux limited sample of X-ray clusters at $0.35 = \alpha \mu + \beta$, with $\mu = \ln (M_{200c}/M_{\mathrm{piv}})$, and $M_{\mathrm{piv}} = 10^{14.81} M_{\odot}$. We find a slope $\alpha = 0.49^{+0.20}_{-0.15}$, normalization $ \exp(\beta) = 84.0^{+9.2}_{-14.8}$ and $\sigma_{\ln \lambda | \mu} = 0.17^{+0.13}_{-0.09}$ using CFHT richness estimates. In comparison to other weak lensing richness-mass relations, we find the normalization of the richness statistically agreeing with the normalization of other scaling relations from a broad redshift range ($0.0<z<0.65$) and with different cluster selection (X-ray, Sun…

COSMOLOGICAL CONSTRAINTSCosmology and Nongalactic Astrophysics (astro-ph.CO)FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsLambdaPROFILE01 natural sciences114 Physical sciencesgravitational lensing: weakMAXBCGweak [gravitational lensing]0103 physical sciencesLARGE-SCALE STRUCTUREclusters: general [galaxies]PROBE010303 astronomy & astrophysicsWeak gravitational lensingGalaxy clusterLOCUSSPhysicsTEMPERATURE RELATION010308 nuclear & particles physicsAstronomy and Astrophysicsobservations [cosmology]RedshiftREDUCTIONSpace and Planetary Sciencegravitational lensing: weak; galaxies: clusters: general; cosmology: observationsgalaxies: clusters: generalcosmology: observationsGIANTSGALAXY CLUSTERS[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astrophysics - Cosmology and Nongalactic Astrophysics
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Holocene climate variability in Sicily from a discontinuous stalagmite record and the Mesolithic to Neolithic transition

2006

AbstractFabric and stable isotopic composition of a Holocene stalagmite (CR1) from a cave in northern Sicily record changes in paleorainfall in the early Holocene. High δ13C stable isotope values in the calcite deposited from ca. 8500 to ca. 7500 yr ago are interpreted as reflecting periods of high rainfall. The wet phase was interrupted by two periods of multi-century duration characterized by relatively cool and dry winters centered at ca. 8200 and ca. 7500 yr ago, highlighted by low δ13C and δ18O values. A high variability of δ13C values is recorded from ca. 7500 to ca. 6500 yr ago and indicates that the transition from a pluvial early Holocene to the present-day climate conditions was p…

Calcite010506 paleontologygeographygeography.geographical_feature_category010504 meteorology & atmospheric sciencesδ13Cδ18OStable isotope ratioStalagmite01 natural scienceschemistry.chemical_compoundArts and Humanities (miscellaneous)chemistryPluvialClimatologyGeneral Earth and Planetary SciencesPhysical geographyGeologyMesolithicHolocene0105 earth and related environmental sciencesEarth-Surface ProcessesStalagmite Sicily Early Holocene paleorainfall
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Accurate trace element analysis of speleothems and biogenic calcium carbonates by LA-ICP-MS

2012

The high spatial resolution of laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) microanalysis of speleothems and biogenic calcium carbonates makes it possible to improve our understanding of past climatic conditions. However, there are analytical problems associated with this method, such as molecular interferences, elemental fractionation, and mass-load-dependent matrix effects, when using NIST silicate reference glasses for calibration. Our study with a sector-field ICP-MS shows that many masses are affected by interferences, such as 24Mg+ by 48Ca++ or 31P+ by 15N16O+. Elemental fractionation and mass-load-dependent matrix effects have been detected for both 213 and…

CalciteAragoniteAnalytical chemistryTrace elementGeologyFractionationengineering.materialMicroanalysisSilicatechemistry.chemical_compoundCalcium carbonatechemistryGeochemistry and PetrologyengineeringGeologyRefractory (planetary science)Chemical Geology
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Bulk composition of northern African dust and its source sediments — A compilation

2013

Abstract This paper presents a review of bulk compositional data of northern African dust and its potential source sediments and includes elemental, isotope and mineralogical data. Northern African dust represents about one half of the total global atmospheric mineral dust burden, and its uplift, transport and deposition have strong impacts on climate and various terrestrial and marine ecosystems. The chemical data set shows, that an ‘average northern African dust’ exhibits comparable Si, Fe and Mn contents with respect to the average composition of the upper continental crust, is slightly depleted in the alkali metals K and Na, and enriched in Ti and P. However, the complete data set yield…

CalciteContinental crustGeochemistryMineralogyengineering.materialMineral dustchemistry.chemical_compoundDeposition (aerosol physics)chemistryIlliteengineeringGeneral Earth and Planetary SciencesCarbonateQuaternaryCompositional dataGeologyEarth-Science Reviews
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Modelling the δ18O value of cave drip water and speleothem calcite

2010

Abstract Stable isotope signals recorded in speleothems have provided important insights about past climate variability in recent years. Quantitative reconstruction of mean annual temperature and the amount of precipitation, however, remains difficult because the stable isotope signals are influenced by various processes. Here we present a drip water model, which shows how these climate parameters affect the oxygen isotope signal of cave drip water. In the model the dependence of the δ 18 O value of drip water on mean annual temperature is established by correlation to the amount of winter precipitation and winter temperature. Application of the model to two caves in western Germany reveals…

CalciteHydrologygeographygeography.geographical_feature_categoryStable isotope ratioδ18OSpeleothemStalagmiteOxygen isotope ratio cycleAtmospheric sciencesIsotopes of oxygenchemistry.chemical_compoundGeophysicsIsotope fractionationchemistrySpace and Planetary ScienceGeochemistry and PetrologyEarth and Planetary Sciences (miscellaneous)GeologyEarth and Planetary Science Letters
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Textural features and isotope geochemistry of the Scillato travertine (north-central Sicily): genetic implications.

2015

The travertine deposit, outcropping near the Scillato town (north-central Sicily), was originated by precipitation of calcium carbonate from the Scillato springs, documented as bicarbonate-enriched waters due to dissolution of the Madonie mountains carbonate rocks. This deposit is today well represented by the Travertine Cave, essentially constituted by stalactites and stalagmites in which travertine typically appears laminated with alternation of light and dark laminae. Mineralogical analysis have revealed the almost exclusive presence of calcite and observation under the polarized-light microscope showed different textural features, like presence of debris and porous portions, micritic po…

Calcitegeographygeography.geographical_feature_categoryMineralogyGeologyStalagmiteSedimentary depositional environmentchemistry.chemical_compoundCalcium carbonatechemistryCaveTufaIsotope geochemistryGeneral Earth and Planetary SciencesCarbonate rockwaterfall tufa speleothems stable carbon and oxygen isotopes microbial activityGeology
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Origin of clay minerals in soils on pyroclastic deposits in the island of Lipari (Italy)

2005

The island of Lipari (Italy) is characterized by calc-alkaline to potassic volcanism and a Mediterranean-type climate. The mineralogical and chemical features of two different soil profiles with ages of 92,000 and 10,000–40,000 y, respectively, have been investigated. There were no Andisols, but Vitric and Vertic Cambisols have developed at both sites. Although the morphology of the soils was similar, remarkable differences in the clay mineralogy between the two sites were observed. The site with the Vitric Cambisol was associated with the weathering sequence: glass → halloysite → kaolinite or interstratified kaolinite-2:1 clay minerals. Both sites had smectite in the clay fraction and, to …

CambisolGeochemistrySoil ScienceMineralogyWeatheringAndisols geochemistry montmorillonite glasses kaolinite sheet silicates Italy Cambisols clay mineralogy Europe silicates soils halloysite Lipari Islands clay minerals igneous rocks Lipari Island smectite metasomatism weathering Sicily Italy volcanic rocks Southern Europeengineering.materialHalloysitechemistry.chemical_compoundMontmorillonitechemistrySettore AGR/14 - PedologiaGeochemistry and PetrologySoil waterEarth and Planetary Sciences (miscellaneous)engineeringSoil horizonKaoliniteClay mineralsGeologyWater Science and Technologyclays and clay minerals
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