Search results for " Active"

showing 10 items of 533 documents

Probing the Internal Structure of Magnetized, Relativistic Jets with Numerical Simulations

2016

From an observational point of view, unveiling the physical processes behind the nature of the jets emanating from radio-loud AGN demands the resolution of the structure across the jet with the highest angular resolutions. Relying on a magneto-fluid dynamical description, numerical simulations can help to characterize the internal structure of jets (transversal structure, magnetic field structure, internal shocks, etc.). In the first part of the paper, we shall discuss equilibrium models of magnetized, relativistic, infinite, axisymmetric jets with rotation propagating through a homogeneous, static, unmagnetized ambient medium. Then, these transversal equilibrium profiles will be used to bu…

PhysicsShock waveJet (fluid)Internal energyMagnetic energyMHDlcsh:Astronomy010308 nuclear & particles physicsAstrophysics::High Energy Astrophysical Phenomenagalaxies: activeAstronomy and Astrophysicsshock wavesgalaxies: jets01 natural sciencesmethods: numericalComputational physicsMagnetic fieldlcsh:QB1-991galaxies: active; galaxies: jets; methods: numerical; MHD; shock wavesRelativistic beamingClassical mechanicsAstrophysical jet0103 physical sciencesMagnetohydrodynamics010303 astronomy & astrophysicsGalaxies
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Calibration of Cholesky Auxiliary Basis Sets for Multiconfigurational Perturbation Theory Calculations of Excitation Energies

2010

The accuracy of auxiliary basis sets derived from Cholesky decomposition of two-electron integrals is assessed for excitation energies calculated at the state-average complete active space self-consistent field (CASSCF) and multiconfigurational second order perturbation theory (CASPT2) levels of theory using segmented as well as generally contracted atomic orbital basis sets. Based on 196 valence excitations in 26 organic molecules and 72 Rydberg excitations in 3 organic molecules, the results show that Cholesky auxiliary basis sets can be used without compromising the accuracy of the multiconfigurational methods. Specifically, with a decomposition threshold of 10(-4) au, the mean error due…

PhysicsValence (chemistry)Mean squared errorComputer Science Applicationssymbols.namesakeAtomic orbitalRydberg formulasymbolsComplete active spacePhysical and Theoretical ChemistryAtomic physicsBasis setExcitationCholesky decompositionJournal of Chemical Theory and Computation
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The XMM-Newton survey of the ELAIS-S1 field

2006

We have surveyed with XMM-Newton the central ~0.6 deg2 region of the ELAIS-S1 field down to flux limits of ~5.5X10-16 cgs (0.5-2 keV, S band), ~2X10-15 cgs (2-10 keV, H band), and ~4X10-15 cgs (5-10 keV, HH band). We detect a total of 478 sources, 395 and 205 of which detected in the S and H bands respectively. We identified 7 clearly extended sources and estimated their redshift through X-ray spectral fits with thermal models. In four cases the redshift is consistent with z=0.4. We have computed the angular correlation function of the sources in the S and H bands, finding best fit correlation angles theta_0=5.2+/-3.8 arcsec and theta_0=12.8+/-7.8 arcsec respectively. A rough estimate of th…

PhysicsX-rays : galaxieField (physics)galaxies : activeAstrophysics (astro-ph)FOS: Physical sciencesFluxAstronomy and AstrophysicsAstrophysicsH bandAstrophysicsRedshiftDistribution (mathematics)Space and Planetary ScienceRange (statistics)Relative densitylarge-scale structure of UniverseS bandAstronomy & Astrophysics
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Multiband Photometry of the Blazar PKS 0537-441: A Major Active State in December 2004 - March 2005

2005

Multiband VRIJHK photometry of the Blazar PKS 0537-441 obtained with the REM telescope from December 2004 to March 2005 is presented. A major period of activity is found with more than four magnitudes variability in the V filter in 50 days and of 2.5 in 10 days. In intensity and duration the activity is similar to that of 1972 reported by Eggen (1973), but it is much better documented. No clear evidence of variability on time-scale of minutes is found. The spectral energy distribution is roughly described by a power-law, with the weaker state being the softer.

Physicsgalaxies: active; galaxies: BL Lacertae objects: PKS 0537-441galaxies: activeAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicslaw.inventionTelescopePhotometry (astronomy)galaxies: BL Lacertae objects: PKS 0537-441Space and Planetary Sciencelawgalaxies: active ; galaxies: BL Lacertae objects: PKS 0537-441active [galaxies]Spectral energy distributionActive stateBlazarBL Lacertae objects: PKS 0537-441 [galaxies]:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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XMM-Newton First-Light Observations of the Hickson Galaxy Group 16

2000

This paper presents the XMM-Newton first-light observations of the Hickson-16 compact group of galaxies. Groups are possibly the oldest large-scale structures in the Universe, pre-dating clusters of galaxies, and are highly evolved. This group of small galaxies, at a redshift of 0.0132 (or 80 Mpc) is exceptional in the having the highest concentration of starburst or AGN activity in the nearby Universe. So it is a veritable laboratory for the study of the relationship between galaxy interactions and nuclear activity. Previous optical emission line studies indicated a strong ionising continuum in the galaxies, but its origin, whether from starbursts, or AGN, was unclear. Combined imaging and…

Physicsmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Continuum (design consultancy)FOS: Physical sciencesAstronomy and AstrophysicsGalaxies: activeAstrophysicsFirst lightAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxy mergerAstrophysicsGalaxyUniverseRedshiftCompact groupSpace and Planetary ScienceGalaxy groupGalaxies: starburstX-rays: galaxieAstrophysics::Galaxy Astrophysicsmedia_common
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Millimeter VLBI of NGC 1052: Dynamics

2016

The LINER galaxy NGC 1052 is an ideal target to study the innermost regions of active galactic nuclei (AGN), given its close distance of about 20 Mpc. The source was observed at 29 epochs from 2005 to 2009 with the Very Long Baseline Array (VLBA) at 43 GHz. Here, we present a kinematic study of its twin-jet system from a subset of 9 epochs at 43 GHz carried out in 2005 and 2006, finding a bright central feature as the dynamic center. The resulting mean velocities of β = v / c = 0 . 46 ± 0 . 08 and β = 0 . 69 ± 0 . 02 for the western and eastern jet, respectively, give hints towards higher velocities in the eastern jet.

Physicsradio continuum: galaxiesJet (fluid)Active galactic nucleusgalaxies: active; galaxies: nuclei; galaxies: jets; radio continuum: galaxies010308 nuclear & particles physicslcsh:Astronomygalaxies: activeAstronomyAstronomy and AstrophysicsAstrophysicsKinematicsgalaxies: jetsDisc galaxy01 natural sciencesGalaxylcsh:QB1-9910103 physical sciencesVery-long-baseline interferometryMillimetergalaxies: nuclei010303 astronomy & astrophysicsVery Long Baseline ArrayGalaxies; Volume 4; Issue 4; Pages: 48
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ChemInform Abstract: Flexible Synthesis of Planar Chiral Azoninones and Optically Active Indolizidinones.

2015

PlanarChemistryOrganic chemistryGeneral MedicineOptically activeCombinatorial chemistryChemInform
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Combining hectometric and decametric satellite observations to provide near real time decametric FAPAR product

2017

Abstract A wide range of ecological, agricultural, hydrological and meteorological applications at local to regional scales requires decametric biophysical data. However, before the launch of SENTINEL-2A, only few decametric products are produced and most of them remain limited by the small number of available observations, mostly due to a moderate revisit frequency combined with cloud occurrence. Conversely, kilometric and hectometric biophysical products are now widely available with almost complete and continuous coverage, but the associated spatial resolution limits the application over heterogeneous landscapes. The objective of this study is to combine unfrequent decametric spatial res…

Point spread functionanalyse de données010504 meteorology & atmospheric sciencesMeteorology[SDV]Life Sciences [q-bio]Real-time computingdata analysis0211 other engineering and technologiesSoil Science02 engineering and technology01 natural sciencesGEOV3Range (statistics)Landsat-8FAPARComputers in Earth Sciencestemps réelImage resolutionphotosynthetically active radiation021101 geological & geomatics engineering0105 earth and related environmental sciencesRemote sensinganalyse temporellereal timePixelrayonnement photosynthétiquement actifGeologyFunction (mathematics)15. Life on landData fusionSensor fusionDecametricHectometric13. Climate actionPhotosynthetically active radiationtime analysisEnvironmental scienceSatelliteNear real timeobservation satellite
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Human Drug Pollution in the Aquatic System: The Biochemical Responses of Danio rerio Adults

2021

Simple Summary The release of medicinal products for human use in the aquatic environment is now a serious problem, and can be fatal for the organisms that live there. Danio rerio is a freshwater fish that provides the possibility to study the effects of these pollutants on the health of aquatic organisms. The results of the various existing scientific studies are scarce and conflicting. Here, we review the scientific studies that have analyzed these effects, highlighting that the impacts of drugs are evident in the biochemical responses of these animals. Abstract To date, drug pollution in aquatic systems is an urgent issue, and Danio rerio is a model organism to study the toxicological ef…

PollutantPollutionoxidative streGeneral Immunology and MicrobiologybiologyQH301-705.5media_common.quotation_subjectDanioReviewcortisolbiology.organism_classificationzebrafishGeneral Biochemistry Genetics and Molecular Biologyimmune responseenzymeDrug concentrationpharmaceutically active compounds (PhAC)Environmental healthoxidative stressDrug pollutionBiology (General)General Agricultural and Biological SciencesTotal proteinmedia_commonBiology
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Multi-Alkenylsilsesquioxanes as Comonomers and Active Species Modifiers of Metallocene Catalyst in Copolymerization with Ethylene.

2018

The copolymers of ethylene (E) with open-caged iso-butyl-substituted tri-alkenyl-silsesquioxanes (POSS-6-3 and POSS-10-3) and phenyl-substituted tetra-alkenyl-silsesquioxane (POSS-10-4) were synthesized by copolymerization over the ansa-metallocene catalyst. The influence of the kind of silsesquioxane and of the copolymerization conditions on the reaction performance and on the properties of the copolymers was studied. In the case of copolymerization of E/POSS-6-3, the positive comonomer effect was observed, which was associated with the influence of POSS-6-3 on transformation of the bimetallic ion pair to the active catalytic species. Functionality of silsesquioxanes and polymerization par…

Polymers and Plastics02 engineering and technologyPost-metallocene catalyst010402 general chemistry01 natural sciencesArticlelcsh:QD241-441chemistry.chemical_compoundlcsh:Organic chemistryPolymer chemistryCopolymerethylenecrosslinkingchemistry.chemical_classificationmetalloceneComonomerGeneral ChemistryPolymer021001 nanoscience & nanotechnologySilsesquioxaneethylene; polyhedral oligomeric silsesquioxanes (POSS); copolymerization; metallocene; crosslinking; active site modifier0104 chemical sciencesactive site modifiercopolymerizationchemistryPolymerization0210 nano-technologyGlass transitionMetallocenepolyhedral oligomeric silsesquioxanes (POSS)Polymers
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