Search results for " chemical evolution"

showing 5 items of 5 documents

ORIGIN: metal creation and evolution from the cosmic dawn

2012

Herder, Jan-Willem den et al.

HOT INTERGALACTIC MEDIUMUNIVERSEChemical evolutionMission7. Clean energy01 natural sciencesSpectral lineSettore FIS/05 - Astronomia E Astrofisica010303 astronomy & astrophysicsmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)NUCLEOSYNTHESISCOSMIC cancer databaseClusters of galaxiesSatellite MissionEpoch (reference date)Astrophysics::Instrumentation and Methods for AstrophysicsFORESTGALAXIESGamma-ray burstsAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaX-ray Mission Gamma-ray bursts Clusters of galaxies Warm-hot intergalactic medium Chemical evolutionWarm-hot intergalactic mediumAstrophysics - Cosmology and Nongalactic AstrophysicsAstrophysics and AstronomyStructure formationCosmology and Nongalactic Astrophysics (astro-ph.CO)Clusters of galaxiemedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaREDSHIFTFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsX-ray Mission Gamma-ray bursts Clusters of galaxies Warm-hot intergalactic medium Chemical evolutionABSORPTION-SPECTRA010309 opticsX-rayYIELDS0103 physical sciencesGamma-ray burstInstrumentation and Methods for Astrophysics (astro-ph.IM)X-ray; Mission; Gamma-ray bursts; Clusters of galaxies; Warm-hot intergalactic medium; Chemical evolutionAstronomyAstronomy and AstrophysicsRedshiftGalaxyUniverse13. Climate actionChemical evolution; Clusters of galaxies; Gamma-ray bursts; Mission; Warm-hot intergalactic medium; X-ray; Astronomy and Astrophysics; Space and Planetary ScienceSpace and Planetary ScienceGamma-ray burstCLUSTERSExperimental Astronomy
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The Hamburg/ESO R-process Enhanced Star survey (HERES):XI. The highly r-process-enhanced star CS 29497-004

2017

We report an abundance analysis for the highly r-process-enhanced (r-II) star CS 29497-004, a very metal-poor giant with Teff = 5013K and [Fe/H]=-2.85, whose nature was initially discovered in the course of the HERES project. Our analysis is based on high signal-to-noise, high-resolution (R~75000) VLT/UVES spectra and MARCS model atmospheres under the assumption of local thermodynamic equilibrium, and obtains abundance measurements for a total of 46 elements, 31 of which are neutron-capture elements. As is the case for the other 25 r-II stars currently known, the heavy-element abundance pattern of CS 29497-004 well-matches a scaled Solar System second peak r-process-element abundance patter…

MODEL ATMOSPHERESSolar SystemPopulation II [stars]Thermodynamic equilibriumMETAL-POOR STARSFOS: Physical sciencesAstrophysicsStar (graph theory)01 natural sciences7. Clean energySpectral lineGalactic halochemically peculiar [stars]CORE-COLLAPSE SUPERNOVAELABORATORY TRANSITION-PROBABILITIES0103 physical sciencesEXPERIMENTAL OSCILLATOR-STRENGTHShalo [Galaxy]NeutronEARLY GALAXY010306 general physics010303 astronomy & astrophysicsComputingMilieux_MISCELLANEOUSSolar and Stellar Astrophysics (astro-ph.SR)PhysicsPROCESS-RICHGALACTIC CHEMICAL EVOLUTIONAstronomy and Astrophysicsindividual: CS 29497-004 [stars][PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Astrophysics - Astrophysics of Galaxiesabundances [stars]StarsHIGH-ENTROPY-WIND[PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Astrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)r-processNEUTRON-CAPTURE
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Rapid chemical evolution of tropospheric volcanic emissions from Redoubt Volcano, Alaska, based on observations of ozone and halogen-containing gases

2013

Abstract We report results from an observational and modeling study of reactive chemistry in the tropospheric plume emitted by Redoubt Volcano, Alaska. Our measurements include the first observations of Br and I degassing from an Alaskan volcano, the first study of O 3 evolution in a volcanic plume, as well as the first detection of BrO in the plume of a passively degassing Alaskan volcano. This study also represents the first detailed spatially-resolved comparison of measured and modeled O 3 depletion in a volcanic plume. The composition of the plume was measured on June 20, 2010 using base-treated filter packs (for F, Cl, Br, I, and S) at the crater rim and by an instrumented fixed-wing a…

Sub arctic troposphereReactive halogenOzone010504 meteorology & atmospheric sciencesChemical evolutionBromine monoxide; Chemical evolution; Ozone depletion; Reactive halogen; Sub arctic troposphere; Volcanic plumeOzone depletion010502 geochemistry & geophysicsAtmospheric sciences01 natural sciencesVolcanic plumeTropospherechemistry.chemical_compoundImpact craterGeochemistry and Petrology0105 earth and related environmental sciencesgeographygeography.geographical_feature_categoryBromine monoxideOzone depletionPlumeGeophysicschemistryVolcano13. Climate actionHalogenGeologyWater vapor
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Ultrahigh- resolving analytics in meteoritic soluble organic matter

2016

International audience; No abstract

[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]non - terrestrial chemical evolution[SDU.ASTR] Sciences of the Universe [physics]/Astrophysics [astro-ph][ SDU.ASTR ] Sciences of the Universe [physics]/Astrophysics [astro-ph]ComputingMilieux_MISCELLANEOUS
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The young hard active Sun: soft X-ray irradiation of tryptophan in water solutions

2010

AbstractThe X-ray emission of the young Sun was much harder and intense than today and might have played a significant role in the evolution of complex organics in protoplanetary environments. We investigate the effects of soft X-rays on tryptophan molecules in aqueous solutions at room temperature. As results of the irradiation experiments we detect several light species indicative of fragmentation, together with large molecular structures such as tryptophan dipeptide and tripeptide. Complexification is more evident in H2O solution than in D2O, probably due to isotopic effects. The abundances of peptides depend on the irradiation dose and decrease with increasing energy deposition. Radical…

amino acidsAqueous solutionDipeptidePhysics and Astronomy (miscellaneous)RadicalastrobiologyTryptophanTripeptidePhotochemistryorigin of lifeX-ray irradiation of amino acidsCrystallographychemistry.chemical_compoundchemistryFragmentation (mass spectrometry)Space and Planetary Scienceamino acids astrobiology chemical evolution origin of life X-ray irradiation of amino acids.Earth and Planetary Sciences (miscellaneous)MoleculeIrradiationchemical evolutionEcology Evolution Behavior and SystematicsInternational Journal of Astrobiology
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