Search results for "Environment"

showing 10 items of 28487 documents

Spectral properties of X-ray bright variable sources in the Taurus Molecular Cloud

2006

We analyze 19 bright variable X-ray sources detected in the XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST), in order to characterize the variations with time of their coronal properties and to derive informations on the X-ray emitting structures. We performed time-resolved spectroscopy of the EPIC PN and MOS spectra of the XEST sources, using a model with one or two thermal components, and we used the time evolution of the temperatures and emission measures during the decay phase of flares to derive the size of the flaring loops. The light curves of the selected sources show different types of variability: flares, long-lasting decay or rise through the whole observation, sl…

stars : pre-main sequence010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaX-rays : starsFOS: Physical sciencesFluxAstrophysicsAstrophysics01 natural sciences7. Clean energySpectral linelaw.inventionlaw0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsSpectroscopy010303 astronomy & astrophysics0105 earth and related environmental sciencesPhysicsMolecular cloudAstrophysics (astro-ph)Astronomy and Astrophysicsstars : late-typeRadiusPlasmaLight curve13. Climate actionSpace and Planetary Sciencestars : coronaeFlare
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Stochastic gravito-inertial modes discovered by CoRoT in the hot Be star HD 51452

2012

International audience; Context. Be stars are rapidly rotating stars with a circumstellar decretion disk. They usually undergo pressure and/or gravity pulsation modes excited by the κ-mechanism, i.e. an effect of the opacity of iron-peak elements in the envelope of the star. In the Milky Way, p-modes are observed in stars that are hotter than or equal to the B3 spectral type, while g-modes are observed at the B2 spectral type and cooler. Aims. We observed a B0IVe star, HD 51452, with the high-precision, high-cadence photometric CoRoT satellite and high-resolution, ground-based HARPS and SOPHIE spectrographs to study its pulsations in great detail. We also used the lower resolution spectra a…

starsBe -stars010504 meteorology & atmospheric sciencesBe starK-type main-sequence staroscillations -starsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsrotation01 natural sciences0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsStellar structureindividual010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciences[PHYS]Physics [physics]PhysicsASTROFÍSICA ESTELARStellar rotationFlare starAstronomyAstronomy and AstrophysicsLight curveESPECTROSCOPIAHD 51452 -starsStarsT Tauri star13. Climate actionSpace and Planetary ScienceAstrophysics::Earth and Planetary Astrophysicsemission-line[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
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Chemical Cartography with APOGEE: Multi-element Abundance Ratios

2019

We map the trends of elemental abundance ratios across the Galactic disk, spanning R = 3-15 kpc and midplane distance |Z|= 0-2 kpc, for 15 elements in a sample of 20,485 stars measured by the SDSS/APOGEE survey (O, Na, Mg, Al, Si, P, S, K, Ca, V, Cr, Mn, Fe, Co, Ni). Adopting Mg rather than Fe as our reference element, and separating stars into two populations based on [Fe/Mg], we find that the median trends of [X/Mg] vs. [Mg/H] in each population are nearly independent of location in the Galaxy. The full multi-element cartography can be summarized by combining these nearly universal median sequences with our measured metallicity distribution functions and the relative proportions of the lo…

stars: abundances010504 meteorology & atmospheric sciencesMilky WayMetallicityPopulationFOS: Physical sciences01 natural sciencesGalaxy: diskStellar nucleosynthesisNucleosynthesis0103 physical scienceseducation010303 astronomy & astrophysicsnuclear reactions0105 earth and related environmental sciencesPhysicseducation.field_of_studyabundancesnucleosynthesisAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesGalaxySupernova13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Galaxy: abundancesSupernova nucleosynthesis[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]CartographyThe Astrophysical Journal
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The Gaia-ESO Survey: impact of extra mixing on C and N abundances of giant stars

2018

The GES survey using FLAMES at the VLT has obtained high-resolution UVES spectra for a large number of giant stars, allowing a determination of the abundances of the key chemical elements C and N at their surface. The surface abundances of these chemical species are well-known to change in stars during their evolution on the red giant branch after the first dredge-up episod, as a result of extra-mixing phenomena. We investigate the effects of thermohaline mixing on C and N abundances using the first comparison between the GES [C/N] determinations with simulations of the observed fields using a model of stellar population synthesis. We explore the effects of thermohaline mixing on the chemic…

stars: abundances010504 meteorology & atmospheric sciencesStellar populationMetallicityFOS: Physical sciencesabundances ; stars: evolution ; galaxy: stellar content ; galaxy: abundances ; astrophysics - solar and stellar astrophysics [stars]AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstronomi astrofysik och kosmologi0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsstellar content [Galaxy]Astronomy Astrophysics and Cosmologystars: evolution14. Life underwater010303 astronomy & astrophysicsStellar evolutionSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsGalaxy: stellar contentabundances [Galaxy]Astronomy and AstrophysicsGiant starRed-giant branchabundances [stars]StarsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceGlobular clusterevolution [stars]Galaxy: abundancesAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Open cluster
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IEL.21-22-Unit 3. The application of International Environmental Law

2022

International Environmental Law. Unit 3. The Application of International Environmental Law. Powerpoint of the Academic course 2021-2022. 15. UNIT 3.-THE APPLICATION OF INTERNATIONAL ENVIRONMENTAL LAW. 1. General aspects: control procedures and bodies - 2. International liability in international environmental law: (a) general aspects; (b) liability for unlawful acts and international environmental crime; (c) liability of States for environmental damage resulting from acts not prohibited by international law - 3. Peaceful settlement of international disputes concerning the protection of the environment.

states liabilityUNESCO::CIENCIAS JURÍDICAS Y DERECHOinternational environmental protectionstates responsibility
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Using uncertain preferential information from stakeholders to assess the acceptability of alternative forest management plans

2017

In forest management planning, participatory planning processes are often encouraged as a means to acquire relevant information and to enhance the stakeholders' acceptability of alternative plans. This requires the aggregation of the stakeholders' preferences that can be done in a wide variety of manners. The aggregation process strives to reduce the information into a single set of preferences that simplifies the information and allows for the use of discrete decision support tools. Depending on how the preferences are aggregated, a wide range of plan rankings can emerge. Although this range of ranking complicates the issue of plan selection, it does highlight the uncertainty involved in a…

stochastic multicriteria acceptability analysisstochastic preferencesComputer scienceStrategy and Managementpäätöksentekostokastinen monikriteerinen arvostusanalyysiForest management0211 other engineering and technologiesGeneral Decision Sciences02 engineering and technologypairwise comparisonsstochastic programminggroup decision makingsidosryhmätryhmätEnvironmental planning040101 forestryStochastic multicriteria acceptability analysis021103 operations researchbusiness.industryEnvironmental resource management04 agricultural and veterinary sciences15. Life on landStochastic programmingGroup decision-makingta11810401 agriculture forestry and fisheriesPairwise comparisonmetsänhoitobusinessosallistava suunnitteluJournal of Multi-Criteria Decision Analysis
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Regulating role of lumbricid macrofauna in Atrazine biodegradation in temperate cropped soil.

2004

communication oraleFR2116communication orale

stomatognathic diseasesInformationSystems_MODELSANDPRINCIPLESComputingMilieux_THECOMPUTINGPROFESSIONGeneralLiterature_INTRODUCTORYANDSURVEYComputingMilieux_COMPUTERSANDEDUCATION[ SDU.ENVI ] Sciences of the Universe [physics]/Continental interfaces environment[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environment[SDU.ENVI] Sciences of the Universe [physics]/Continental interfaces environment
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Interactions biotiques entre macrofaune lombricienne et les communautés microbiennes, indigènes et bioaugmentées, dégradant l'atrazine en sol tempéré.

2004

communication oraleFR2116communication orale

stomatognathic diseasesInformationSystems_MODELSANDPRINCIPLESComputingMilieux_THECOMPUTINGPROFESSIONGeneralLiterature_INTRODUCTORYANDSURVEY[ SDU.ENVI ] Sciences of the Universe [physics]/Continental interfaces environmentComputingMilieux_COMPUTERSANDEDUCATION[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environment[SDU.ENVI] Sciences of the Universe [physics]/Continental interfaces environment
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Biodégradation de l'atrazine en sols tempérés : rôle régulateur d'un modèle d'interaction biotique macrofaune/bactérie.

2004

communication orale

stomatognathic diseasesInformationSystems_MODELSANDPRINCIPLESComputingMilieux_THECOMPUTINGPROFESSIONGeneralLiterature_INTRODUCTORYANDSURVEY[ SDU.ENVI ] Sciences of the Universe [physics]/Continental interfaces environmentComputingMilieux_COMPUTERSANDEDUCATION[SDU.ENVI]Sciences of the Universe [physics]/Continental interfaces environment[SDU.ENVI] Sciences of the Universe [physics]/Continental interfaces environment
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Effects of integrating a bioethanol production process to a kraft pulp mill

2010

Abstract The integration of an ethanol production process based on prehydrolysis of softwood chips to a kraft pulp mill is discussed. A simulation model of this biorefinery has been created with WinGEMS simulation software to calculate the mass and energy balances of the biorefinery and to examine the effects of the integration on the operation of the pulp mill. Integrating the prehydrolysis process to the modeled pulp mill producing 1000 Adt/day of pine pulp would increase the wood consumption by 16%. With the increased wood consumption, 40 t/day of ethanol could be produced, and the excess power production could be increased by 460 MWh/day. The integration of the ethanol production proces…

stomatognathic systemKraft processBiofuelSoda pulpingtechnology industry and agriculturefood and beveragesEnvironmental scienceMillGeneral Materials ScienceForestryPulp and paper industrycomplex mixturesKraft paperNordic Pulp & Paper Research Journal
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