Search results for "AE"

showing 10 items of 28636 documents

Matter Mixing in Aspherical Core-collapse Supernovae: Three-dimensional Simulations with Single Star and Binary Merger Progenitor Models for SN 1987A

2019

We perform three-dimensional hydrodynamic simulations of aspherical core-collapse supernovae focusing on the matter mixing in SN 1987A. The impacts of four progenitor (pre-supernova) models and parameterized aspherical explosions are investigated. The four pre-supernova models include a blue supergiant (BSG) model based on a slow merger scenario developed recently for the progenitor of SN 1987A (Urushibata et al. 2018). The others are a BSG model based on a single star evolution and two red supergiant (RSG) models. Among the investigated explosion (simulation) models, a model with the binary merger progenitor model and with an asymmetric bipolar-like explosion, which invokes a jetlike explo…

010504 meteorology & atmospheric sciencesSupergiant starAstrophysics::High Energy Astrophysical PhenomenaBinary numberchemistry.chemical_elementNeutron starFOS: Physical sciencesHydrodynamical simulationAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesCore-collapse supernovaeAstrophysics::Solar and Stellar AstrophysicsRed supergiant010303 astronomy & astrophysicsMixing (physics)HeliumStellar evolutionary modelSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesLine (formation)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astronomy and AstrophysicsSupernova dynamicSupernovaNeutron starchemistryAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceExplosive nucleosynthesisSupergiantAstrophysics - High Energy Astrophysical Phenomena
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Results from DROXO IV. EXTraS discovery of an X-ray flare from the Class I protostar candidate ISO-Oph 85

2016

X-ray emission from Young Stellar Objects (YSOs) is crucial to understand star formation. A very limited amount of X-ray results is available for the protostellar (ClassI) phase. A systematic search of transient X-ray phenomena combined with a careful evaluation of the evolutionary stage offer a widely unexplored window to our understanding of YSOs X-ray properties. Within the EXTraS project, a search for transients and variability in the whole XMM-Newton archive, we discover transient X-ray emission consistent with ISO-Oph 85, a strongly embedded YSO in the rho Ophiuchi region, not detected in previous time-averaged X-ray studies. We extract an X-ray light curve for the flare and determine…

010504 meteorology & atmospheric sciencesYoung stellar objectAstrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesflares; X-rayslaw.inventionPhotometry (optics)law0103 physical sciencesProtostarAstrophysics::Solar and Stellar Astrophysicseducation010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencescoronaePhysicseducation.field_of_studystars: protostarsStar formationactivityAstronomy and AstrophysicsLight curveAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceSpectral energy distributionAstrophysics::Earth and Planetary AstrophysicsFlare
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Deep X-ray view of the Class I YSO Elias 29 with XMM-Newton and NuSTAR

2019

[Abridged] We investigated the X-ray characteristics of the Class I YSO Elias 29 with joint XMM-Newton and NuSTAR observations of 300 ks and 450 ks, respectively. These are the first observations of a very young (<1 Myr) stellar object in a band encompassing simultaneously both soft and hard X-rays. In addition to the hot Fe complex at 6.7 keV, we observed fluorescent emission from Fe at $\sim6.4$ keV, confirming the previous findings. The line at 6.4 keV is detected during quiescent and flaring states and its flux is variable. The equivalent width is found varying in the $\approx 0.15--0.5$ keV range. These values make unrealistic a simple model with a centrally illuminated disk and sug…

010504 meteorology & atmospheric sciencesYoung stellar objectAstrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionSettore FIS/05 - Astronomia E Astrofisicalaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicseducation010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesLine (formation)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)education.field_of_studyStar formationAstronomy and AstrophysicsCoronaAccretion (astrophysics)Astrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomenastars:activity–stars:coronae–stars:pre-mainsequence–stars:formation–stars:flareEquivalent widthFlare
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The Early-Cambrian Boho volcano of the El Graara massif, Morocco: Petrology, geodynamic setting and coeval sedimentation

2006

15 pages; International audience; A major volcanic episode is recorded across the Neoproterozoic-Cambrian transition in the Moroccan Anti-Atlas. Several volcanic cones are still preserved in the El Graara massif, laterally correlatable with volcanic flows dated as Early Cambrian (U/Pb date of 534 ± 10 Ma). Volcanic ashes and flows are interbedded with the uppermost part of the Adoudou dolostones, whereas the best-preserved volcano (the Boho Jbel) is onlapped by the overlying Lie-de-vin strata. Available petro-geochemical data from the Boho volcano suggest an alkaline magmatism probably derived from low-grade melting of a garnet–lherzolite mantle source, followed by fractional crystallizatio…

010504 meteorology & atmospheric sciences[SDE.MCG]Environmental Sciences/Global ChangesGeochemistrySlope apron[ SDU.STU.VO ] Sciences of the Universe [physics]/Earth Sciences/Volcanology010502 geochemistry & geophysics[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/StratigraphySyenites01 natural sciencesDiagenesisLower CambrianBreccia[SDU.STU.VO]Sciences of the Universe [physics]/Earth Sciences/VolcanologyAlkaline basaltsPetrologySlope aponComputingMilieux_MISCELLANEOUS0105 earth and related environmental sciencesEarth-Surface Processes[ SDU.STU.PG ] Sciences of the Universe [physics]/Earth Sciences/PaleontologyBasaltgeographygeography.geographical_feature_categoryTerrigenous sedimentGeologyMassifDiagenesis[ SDE.MCG ] Environmental Sciences/Global ChangesMoroccoVolcano13. Climate action[SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/StratigraphySubaerial[SDU.STU.PG] Sciences of the Universe [physics]/Earth Sciences/Paleontology[SDU.STU.PG]Sciences of the Universe [physics]/Earth Sciences/PaleontologyVolcanic coneGeology
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The first 40Ar-39Ar date from Oxfordian ammonite-calibrated volcanic layers (bentonites) as a tie-point for the Late Jurassic.

2013

AbstractEight volcanic ash layers, linked to large explosive events caused by subduction-related volcanism from the Vardar Ocean back-arc, interbedded with marine limestones and cherts, have been identified in the Rosso Ammonitico Veronese Formation (northeastern Italy). The thickest ash layer, attributed to the Gregoryceras transversarium ammonite Biozone (Oxfordian Stage), yields a precise and reliable 40Ar–39Ar date of 156.1 ± 0.89 Ma, which is in better agreement with GTS2004 boundaries than with the current GTS2012. This first biostratigraphically well-constrained Oxfordian date is proposed as a new radiometric tie-point to improve the Geologic Time Scale for the Late Jurassic, where a…

010504 meteorology & atmospheric sciences[SDE.MCG]Environmental Sciences/Global ChangesgeochronologyBiozone010502 geochemistry & geophysics[ SDU.STU.ST ] Sciences of the Universe [physics]/Earth Sciences/Stratigraphy01 natural sciencesOxfordianPaleontologyGeologic time scale[SDU.STU.GC]Sciences of the Universe [physics]/Earth Sciences/GeochemistryStage (stratigraphy)0105 earth and related environmental sciencesAmmonitegeographygeography.geographical_feature_categorypalaeovolcanismbentoniteGeology[ SDU.STU.GC ] Sciences of the Universe [physics]/Earth Sciences/Geochemistrylanguage.human_languageJurassic Time Scale[ SDE.MCG ] Environmental Sciences/Global ChangesVolcano[SDU.STU.ST]Sciences of the Universe [physics]/Earth Sciences/StratigraphyGeochronologylanguageRadiometric datingGeologyVolcanic ash
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Trace element behaviour in seawater during Etna's pyroclastic activity in 2001: Concurrent effects of nutrients and formation of alteration minerals

2010

volcanic ash ; trace element leaching ; kinetic experiments ; chlorophyll-alpha; International audience; The eruption of Etna in Sicily on 13 July 2001 marked the most intense activity of the volcano in the last 300 years. The eruption occurred while the oceanographic cruise ANSIC 01 was being conducted to the east of Sicily, presenting a unique opportunity for the investigation of the chemical effects on the marine system during a period of significant (similar to 1 g m(-2)) ash deposition. Comparison of trace element data with measured concentrations from the oceanographic cruise JUVENILE 99, carried out two years before, indicates large enrichments of V. Cr, Mn, Fe, Co, Cu and Pb. We att…

010504 meteorology & atmospheric sciences[SDU.STU]Sciences of the Universe [physics]/Earth SciencesPyroclastic rockMineralogy010502 geochemistry & geophysics01 natural sciencesWater columnGeochemistry and Petrology14. Life underwaterLeaching (agriculture)Kinetic experiment0105 earth and related environmental sciencesgeographygeography.geographical_feature_categoryChlorophyll-αTrace elementGeophysicsDeposition (aerosol physics)Volcano13. Climate actionEnvironmental chemistryTrace element leachingSeawaterVolcanic ashGeologyVolcanic ashJournal of Volcanology and Geothermal Research
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Tectonics of the Northern Bresse region (France) during the Alpine cycle

2003

International audience; Combining fieldwork and surface data, we have reconstructed the Cenozoic structural and tectonic evolution of the Northern Bresse. Analysis of drainage network geometry allowed to detect three major fault zones trending NE-SW, E-W and NW-SE, and smooth folds with NNE trending axes, all corroborated with shallow well data in the graben and fieldwork on edges. Cenozoic paleostress succession was determined through fault slip and calcite twin inversions, taking into account data of relative chronology. A N-S major compression, attributed to the Pyrenean orogenesis, has activated strike-slip faults trending NNE along the western edge and NE-SW in the graben. After a tran…

010504 meteorology & atmospheric sciences[SHS.ARCHEO]Humanities and Social Sciences/Archaeology and PrehistorySketch map010502 geochemistry & geophysics01 natural sciences[SHS]Humanities and Social SciencesPaleontologyBresse grabenMicrotectonicsCompression (geology)0105 earth and related environmental sciencesEarth-Surface Processes[SHS.ARCHEO] Humanities and Social Sciences/Archaeology and PrehistoryDeformation (mechanics)Alpine orogenesisGrabenTectonicsGeophysicsPaleostressesDrainage[SHS] Humanities and Social SciencesQuaternaryCenozoicGeologySeismologyChronology
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Soil erosion in sloping vineyards assessed by using botanical indicators and sediment collectors in the Ruwer-Mosel valley

2016

Steep slopes, erodible soils, rill and ephemeral gullies, compaction due to wheel. traffic and human trampling are common features in vineyards around the world and result in high soil erosion rates. However, little is known about seasonal and spatial variations of soil erosion rates due to factors such as the impact of the vine plantation, harvest, and tillage on the soil redistribution over the long-term temporal scale. The goal of this study is to assess long-term soil erosion rates and the impact of management on sediment and runoff yield by means of Gerlach troughs and a topographical approach based on botanic benchmarks in two paired vineyards with different ages (3 and 35 years) loca…

010504 meteorology & atmospheric sciences[SHS.ARCHEO]Humanities and Social Sciences/Archaeology and PrehistoryVineyard01 natural sciencesVineyard[ SHS.ENVIR ] Humanities and Social Sciences/Environmental studies[ SHS.GEO ] Humanities and Social Sciences/GeographyRuwer-Mosel valleyStock unearthing methodRUSLE0105 earth and related environmental sciences2. Zero hungerHydrologyTopsoilgeographygeography.geographical_feature_categoryEcologyEcology04 agricultural and veterinary sciences[SHS.GEO]Humanities and Social Sciences/Geography15. Life on landBodemfysica en LandbeheerPE&RCRillTillageSoil Physics and Land Management[ SHS.ARCHEO ] Humanities and Social Sciences/Archaeology and Prehistory[SHS.ENVIR]Humanities and Social Sciences/Environmental studiesSoil waterGerlach trough040103 agronomy & agricultureErosionSoil erosion0401 agriculture forestry and fisheriesEnvironmental scienceAnimal Science and ZoologyGerlach trough Stock unearthing methodTramplingSurface runoffAgronomy and Crop Science
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The Chevroches zodiacal cap and its Burgundy relations

2009

AbstractThe excavation of an unexplored secondary agglomeration in Chevroches (France), from 2001 to 2002 has led to the discovery of a bronze dome of a type unknown in the Ancient world. It is inscribed with three lines in Greek transcribing Egyptian and Roman months, and the twelve signs of the Zodiac. This paper presents the first observations and some other finds from similar objects in Burgundy.

010504 meteorology & atmospheric sciences[SHS.ARCHEO]Humanities and Social Sciences/Archaeology and Prehistorymedia_common.quotation_subjectDomeengineering.material01 natural sciencesAstrologyZodiac0103 physical sciencesBronze010303 astronomy & astrophysics0105 earth and related environmental sciencesmedia_commonmechanismsZodiacal light[SHS.ARCHEO] Humanities and Social Sciences/Archaeology and PrehistoryAstronomy and AstrophysicsExcavationArtArchaeologyZodiacSpace and Planetary Science[ SHS.ARCHEO ] Humanities and Social Sciences/Archaeology and PrehistoryengineeringastrologyBurgundyInscribed figure
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A sugar biomarker proxy for assessing terrestrial versus aquatic sedimentary input

2016

Abstract One of the most important and at the same time most challenging issues in paleolimnological research is the differentiation between terrestrial and aquatic sedimentary organic matter (OM). We therefore investigated the relative abundance of the sugars fucose (fuc), arabinose (ara) and xylose (xyl) from various terrestrial and aquatic plants, as well as from algal samples. Algae were characterized by a higher abundance of fucose than vascular plants. Our results and a compilation of data from the literature suggest that fuc/(ara + xyl) and (fuc + xyl)/ara ratios may serve as complementary proxies in paleolimnological studies for distinguishing between terrestrial and aquatic sedimen…

010504 meteorology & atmospheric sciencesbiologyXylose010502 geochemistry & geophysicsbiology.organism_classification01 natural sciencesPaleolimnologyFucosechemistry.chemical_compoundAlgaechemistryGeochemistry and PetrologyAquatic plantBotanySedimentary organic matterSugarRelative species abundance0105 earth and related environmental sciencesOrganic Geochemistry
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