Search results for "nuclei"

showing 10 items of 1273 documents

Sub-milliarcsecond imaging of 3C111

2020

Flares in radio-loud active galactic nuclei (AGNs) are thought to be associated with the injection of fresh plasma into the compact jet base. Such flares are usually strongest and appear earlier at shorter radio wavelengths. Hence, very long baseline interferometry (VLBI) at millimeter (mm)-wavelengths is the best-suited technique for studying the earliest structural changes of compact jets associated with emission flares. Aims. We study the morphological changes of the parsec-scale jet in the nearby (z=0.049) gamma-ray bright radio galaxy 3C 111 following a flare that developed into a major radio outburst in 2007. We analyse three successive observations of 3C 111 at 86 GHz with the Global…

galactic and extragalactic astronomyAstrophysics and AstronomyActive galactic nucleihigh energy astrophysicsPhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxiesobservational astronomyRadio galaxiesPhysics::Space PhysicsAstrophysics::Solar and Stellar AstrophysicsNatural SciencesAstrophysics::Galaxy AstrophysicsVery long baseline interferometry
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MOJAVE. VI. Kinematic analysis of blazar jets

2012

We discuss the jet kinematics of a complete flux-density-limited sample of 135 radio-loud active galactic nuclei (AGNs) resulting from a 13 year program to investigate the structure and evolution of parsec-scale jet phenomena. Our analysis is based on new 2cm Very Long Baseline Array (VLBA) images obtained between 2002 and 2007, but includes our previously published observations made at the same wavelength, and is supplemented by VLBA archive data. In all, we have used 2424 images spanning the years 1994-2007 to study and determine the motions of 526 separate jet features in 127 jets. Cone search capability for table J/AJ/138/1874/agn (AGN sample)

galactic and extragalactic astronomyAstrophysics and AstronomyActive galactic nucleihigh energy astrophysicsRadio sourcesAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic Astrophysicsstellar astronomyCosmologyobservational astronomyBL Lacertae objectsRadio astronomyNatural SciencesQuasarsAstrophysics::Galaxy Astrophysics
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22GHz image of 3C 273

2017

RadioAstron is a 10m orbiting radio telescope mounted on the Spektr-R satellite, launched in 2011, performing Space Very Long Baseline Interferometry (SVLBI) observations supported by a global ground array of radio telescopes. With an apogee of ~350000km, it is offering for the first time the possibility to perform as-resolution imaging in the cm-band. The RadioAstron Active Galactic Nuclei (AGN) polarization Key Science Project (KSP) aims at exploiting the unprecedented angular resolution provided by RadioAstron to study jet launching/collimation and magnetic-field configuration in AGN jets. The targets of our KSP are some of the most powerful blazars in the sky. We present observations at…

galactic and extragalactic astronomyAstrophysics and AstronomyActive galactic nucleihigh energy astrophysicsRadio sourcesPhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsCosmologyobservational astronomyMagnetic fieldsRadio astronomyAstrophysical ProcessesNatural SciencesAstrophysics::Galaxy Astrophysics
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Modelling molecular iodine emissions in a coastal marine environment: The link to new particle formation

2006

International audience; A model of iodine chemistry in the marine boundary layer (MBL) has been used to investigate the impact of daytime coastal emissions of molecular iodine (I2). The model contains a full treatment of gas-phase iodine chemistry, combined with a description of the nucleation and growth, by condensation and coagulation, of iodine oxide nano-particles. In-situ measurements of coastal emissions of I2 made by the broadband cavity ring-down spectroscopy (BBCRDS) and inductively coupled plasma-mass spectrometry (ICP/MS) techniques are presented and compared to long path differential optical absorption spectroscopy (DOAS) observations of I2 at Mace Head, Ireland. Simultaneous me…

homogeneous nucleationspectroscopyAtmospheric ScienceAnalytical chemistryIodine oxideoiochemistrylcsh:ChemistryTropospherechemistry.chemical_compoundCloud condensation nucleiSpectroscopy[SDU.OCEAN]Sciences of the Universe [physics]/Ocean Atmospherepotential influenceChemistryDifferential optical absorption spectroscopyCondensationboundary-layerOzone depletionlcsh:QC1-999ozonelcsh:QD1-999troposphereParticleoxidespectrometer/dk/atira/pure/subjectarea/asjc/1900/1902lcsh:Physics
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Investigation of the p–Σ0 interaction via femtoscopy in pp collisions

2020

This Letter presents the first direct investigation of the p–Σ0 interaction, using the femtoscopy technique in high-multiplicity pp collisions at s=13 TeV measured by the ALICE detector. The Σ0 is reconstructed via the decay channel to Λγ, and the subsequent decay of Λ to pπ−. The photon is detected via the conversion in material to e+e− pairs exploiting the capability of the ALICE detector to measure electrons at low transverse momenta. The measured p–Σ0 correlation indicates a shallow strong interaction. The comparison of the data to several theoretical predictions obtained employing the Correlation Analysis Tool using the Schrödinger Equation (CATS) and the Lednický–Lyuboshits approach s…

hypernucleihyperonsNuclear and High Energy Physicshiukkasfysiikka
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Beta-Decay Half-Lives and Neutron-Emission Probabilities of Very Neutron-Rich Y to Tc Isotopes

1996

Neutron-rich {sub 39}Y to {sub 43}Tc isotopes have been produced by fission of uranium with a 50MeV H{sub 2}{sup +} beam. Beta-decay half-lives, delayed neutron-emission probabilities, and production yields have been measured and compared with theory. Beta decay of 4 new isotopes is reported, and the {beta}-delayed neutron-emission mode has been discovered for 12 isotopes of the elements niobium and technetium. The results compared to quasiparticle random phase approximation predictions indicate the increasing importance of fast {beta} transitions to high-lying states of nuclei with large neutron excess. {copyright} {ital 1996 The American Physical Society.}

inorganic chemicalsPhysicsNUCLEISTABILITYIsotopeFissionNeutron emissionAstrophysics::High Energy Astrophysical PhenomenaNuclear Theorytechnology industry and agriculturePREDICTIONSGeneral Physics and Astronomychemistry.chemical_elementUraniumFISSIONBeta decayYttrium IsotopesNuclear physicschemistryProduction (computer science)NeutronNuclear ExperimentPhysical Review Letters
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The CdCl2 effects on synthetic DNAs encaged in the nanodomains of a cationic water-in-oil microemulsion

2011

The present work is dedicated to the study of the interactions of CdCl(2) with the synthetic polynucleotides polyAT and polyGC confined in the nanoscopic aqueous compartment of the water-in-oil microemulsion CTAB/pentanol/hexane/water, with the goal to mimic in vitro the situation met by the nucleic acids in vivo. In biological structures, in fact, very long strings of nucleic acids are segregated into very small compartments having a radius exceedingly smaller than the length of the encapsulated macromolecule. For comparison, the behaviour of polyGC was also studied in aqueous solutions of matched composition. The conformational and thermal stabilities of both polynucleotides enclosed in t…

inorganic chemicalsnanodomaincadmiumPolynucleotideswater-in-oil microemulsion; cadmium; model polynucleotidesGeneral Physics and AstronomyDissociation (chemistry)model polynucleotideschemistry.chemical_compoundCadmium ChlorideHexanesOrganic chemistryMicroemulsionPhysical and Theoretical ChemistryAqueous solutionconformational transitionCetrimoniumChemistryCationic polymerizationWaterDNAHexaneUV and CD spectroscopiesreverse micelleChemical engineeringwater-in-oil microemulsionPolynucleotideCetrimonium CompoundsNucleic acidCationic w/o microemulsionEmulsionssynthetic polynucleotideOilsMacromolecule
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Measurement of the low-energy antideuteron inelastic cross section

2020

In this Letter, we report the first measurement of the inelastic cross section for antideuteron-nucleus interactions at low particle momenta, covering a range of $0.3 \leq p < 4$ GeV/$c$. The measurement is carried out using p-Pb collisions at a center-of-mass energy per nucleon-nucleon pair of $\sqrt{s_{\rm{NN}}}$ = 5.02 TeV, recorded with the ALICE detector at the CERN LHC and utilizing the detector material as an absorber for antideuterons and antiprotons. The extracted raw primary antiparticle-to-particle ratios are compared to the results from detailed ALICE simulations based on the GEANT4 toolkit for the propagation of antiparticles through the detector material. The analysis of th…

interaction [cosmic radiation]MOMENTUM RANGEAntiparticle:Kjerne- og elementærpartikkelfysikk: 431 [VDP]HadronGeneral Physics and AstronomyPROPAGATIONcosmic radiation: interactionhiukkasfysiikkanucl-ex01 natural sciencesHigh Energy Physics - ExperimentHigh Energy Physics - Experiment (hep-ex)ALICEbenchmarknucleon nucleonHadron-Hadron scattering (experiments)antideuteronmodel: GlauberpropagationAnti-nuclei[PHYS.HEXP]Physics [physics]/High Energy Physics - Experiment [hep-ex]ABSORPTIONAntimatter; heavy ion reactionsNuclear Experiment (nucl-ex)Nuclear ExperimentNuclear Experimenthadron-hadron scatteringNuclear Physics LHC ALICEPhysicsHadron-Hadron scattering (experiments); antinuclei cross sectionsLarge Hadron Colliderp: spectrumheavy ion reactionsPhysicsspectrum [p]VDP::Kjerne- og elementærpartikkelfysikk: 431antinuclei cross sectionsanti-pddc:3. Good healthPRIRODNE ZNANOSTI. Fizika.:Nuclear and elementary particle physics: 431 [VDP]DEUTERONSantimateriaVDP::Nuclear and elementary particle physics: 431COALESCENCEAntimatterGEANTantinucleus: productionydinfysiikkaParticle Physics - ExperimentPB-PB COLLISIONSAntimatterCERN Labinterpretation of experiments: CERN LHC CollFOS: Physical sciences[PHYS.NEXP]Physics [physics]/Nuclear Experiment [nucl-ex]Physics and Astronomy(all)114 Physical sciencesdark matterNuclear physicsMomentumCross section (physics)0103 physical sciencesSCATTERINGddc:530Anti-nuclei; ALICE experiment; hadron-hadron scatteringNuclear Physics - Experimentnumerical calculations010306 general physicsHE-4PB-PB COLLISIONS; LIGHT-NUCLEI; MOMENTUM RANGE; GEV-C; ABSORPTION; HE-4; PROPAGATION; COALESCENCE; SCATTERING; DEUTERONShep-exGlauber [model]low-energy antideuteron ; cross sectionALICE experimentparametrizationantiparticleNATURAL SCIENCES. Physics.LIGHT-NUCLEIGEV-CAntiprotonCERN LHC Coll [interpretation of experiments]Elementary Particles and FieldsHigh Energy Physics::Experimentproduction [antinucleus]Glauber
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15GHz and jet properties of MOJAVE blazars

2013

We investigate the Fermi Large Area Telescope {gamma}-ray and 15GHz Very Long Baseline Array radio properties of a joint {gamma}-ray and radio-selected sample of active galactic nuclei (AGNs) obtained during the first 11 months of the Fermi mission (2008 August 4-2009 July 5). Our sample contains the brightest 173 AGNs in these bands above declination -30{deg} during this period, and thus probes the full range of {gamma}-ray loudness ({gamma}-ray to radio band luminosity ratio) in the bright blazar population. The latter quantity spans at least 4 orders of magnitude, reflecting a wide range of spectral energy distribution (SED) parameters in the bright blazar population. The BL Lac objects,…

interstellar mediumActive galactic nucleigalactic and extragalactic astronomyAstrophysics and AstronomyGamma-ray astronomyhigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSurveysstellar astronomyCosmologyobservational astronomyRadio continuum emissionGamma ray astronomyBL Lacertae objectsRadio astronomyNatural SciencesQuasarsAstrophysics::Galaxy Astrophysics
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1.5Jy MOJAVE AGN sample and 3FGL data

2016

We use the complete MOJAVE 1.5Jy sample of active galactic nuclei (AGNs) to examine the gamma-ray detection statistics of the brightest radio-loud blazars in the northern sky. We find that 23% of these AGNs were not detected above 0.1GeV by the Fermi-LAT during the four-year 3FGL catalog period partly because of an instrumental selection effect and partly due to their lower Doppler boosting factors. Blazars with synchrotron peaks in their spectral energy distributions located below 10^13.4^Hz also tend to have high-energy peaks that lie below the 0.1GeV threshold of the LAT, and are thus less likely to be detected by Fermi. The non-detected AGNs in the 1.5Jy sample also have significantly l…

interstellar mediumActive galactic nucleigalactic and extragalactic astronomyAstrophysics and AstronomyGamma-ray astronomyhigh energy astrophysicsAstrophysics::High Energy Astrophysical PhenomenaPhysicsAstrophysics::Instrumentation and Methods for AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsRedshiftedComputer Science::Digital LibrariesCosmologyobservational astronomyRadio continuum emissionGamma ray astronomyRadio astronomyNatural SciencesAstrophysics::Galaxy Astrophysics
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