Search results for "Astrophysics"

showing 10 items of 8341 documents

Unveiling the environment and faint features of the isolated galaxy CIG 96 with deep optical and HI observations

2018

Context. Asymmetries in atomic hydrogen (HI) in galaxies are often caused by the interaction with close companions, making isolated galaxies an ideal framework to study secular evolution. The AMIGA project has demonstrated that isolated galaxies show the lowest level of asymmetry in their HI integrated profiles compared to even field galaxies, yet some present significant asymmetries. CIG 96 (NGC 864) is a representative case reaching a 16% level. Aims. Our aim is to investigate the HI asymmetries of the spiral galaxy CIG 96 and what processes have triggered the star-forming regions observed in the XUV pseudo-ring. Methods. We performed deep optical observations at CAHA1.23m, CAHA2.2m and V…

galaxies: spiralHIERARCHICAL SATELLITE ACCRETIONmedia_common.quotation_subjectFOS: Physical sciencesAstrophysicsI.01 natural sciences7. Clean energyAsymmetryAMIGA SAMPLElaw.inventionTelescopelaw0103 physical scienceskinematics and dynamics [galaxies]DARK-MATTER SUBSTRUCTURESurface brightness010303 astronomy & astrophysicsStellar evolutionComputingMilieux_MISCELLANEOUSevolution [galaxies]galaxies: kinematics and dynamicsLOPSIDED SPIRAL GALAXIESmedia_commonindividual: NGC 864 [galaxies]Physicsradio lines: galaxiesSpiral galaxy010308 nuclear & particles physicsgalaxies: individual: NGC864Astronomy and AstrophysicsDISK GALAXIESAstrophysics - Astrophysics of GalaxiesAccretion (astrophysics)Galaxygalaxies [radio lines]RINGSTIDAL STREAMspiral [galaxies][SDU]Sciences of the Universe [physics]Space and Planetary ScienceGASAstrophysics of Galaxies (astro-ph.GA)structure [galaxies]galaxies: structureDIGITAL SKY SURVEYCirrusGalaxies: Individual: NGC 864galaxies: evolutionAstronomy & astrophysics
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Searching for differences in Swift's intermediate GRBs

2010

Gamma-ray bursts are usually classified through their high-energy emission into short-duration and long-duration bursts, which presumably reflect two different types of progenitors. However, it has been shown on statistical grounds that a third, intermediate population is needed in this classification scheme, although an extensive study of the properties of this class has so far not been done. The large amount of follow-up studies generated during the Swift era allows us to have a suficient sample to attempt a study of this third population through the properties of their prompt emission and their afterglows. Our study is focused on a sample of GRBs observed by Swift during its first four y…

gamma-rays burst: generalSwiftPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)education.field_of_studyCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstronomy and AstrophysicsClassification schemeAstrophysicsLight curveRedshiftFIS/05 - ASTRONOMIA E ASTROFISICASupernovaSpace and Planetary ScienceThin shellsAstrophysics - High Energy Astrophysical PhenomenaEjectaeducationcomputerAstrophysics - Cosmology and Nongalactic Astrophysicscomputer.programming_language
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Faint γ-ray sources at low redshift: the radio galaxy IC 1531

2018

We present amultiwavelength study of IC 1531 (z=0.02564), an extragalactic radio source associated with the γ -ray object 3FGL J0009.9-3206 and classified as a blazar of uncertain type in the Third Fermi-Large Area Telescope AGN catalog (3LAC). A core-jet structure, visible in radio and X-rays, is enclosed within a ~220 kpc wide radio structure. The morphology and spectral characteristics of the kiloparsec jet in radio and X-rays are typical of Fanaroff-Riley type I galaxies. The analysis of the radio data and optical spectrum and different diagnostic methods based on the optical, infrared, and γ -ray luminosities also support a classification as a low-power RG seen at moderate angles (θ = …

gamma-rays: galaxiesRadio galaxyInfraredGamma-rays: galaxieAstrophysics::High Energy Astrophysical Phenomenagalaxies: activejets [galaxies]AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsGalaxies: jet01 natural sciencesRadio continuum: galaxielaw.inventionTelescopelaw0103 physical sciencesBlazargalaxies: individual: IC 1531010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsradio continuum: galaxies010308 nuclear & particles physicsAstronomy and AstrophysicsAstronomy and Astrophysicgalaxies: jetsGalaxyRedshiftgalaxies [radio continuum]galaxies [gamma-rays]Space and Planetary Scienceactive [galaxies]individual: ic 1531 [galaxies]Spectral energy distributionAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Fermi Gamma-ray Space Telescope
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Acoustic detection of neutrinos in bedrock

2019

We propose to utilize bedrock as a medium for acoustic detection of particle showers following interactions of ultra-high energy neutrinos. With the density of rock three-times larger and the speed of sound four-times larger compared to water, the amplitude of the generated bipolar pressure pulse in rock should be larger by an order of magnitude. Our preliminary simulations confirm that prediction. Higher density of rock also guarantees higher interaction rate for neutrinos. A noticeably longer attenuation length in rock reduces signal dissipation. The Pyh\"asalmi mine has a unique infrastructure and rock conditions to test this idea and, if successful, extend it to a full-size experiment.

geographyPhysics - Instrumentation and Detectorsgeography.geographical_feature_categoryBedrockPhysicsQC1-999neutriinotAttenuation lengthFOS: Physical sciencesGeophysicsInstrumentation and Detectors (physics.ins-det)DissipationHigh Energy Physics - ExperimentPhysics::GeophysicsHigh Energy Physics - Experiment (hep-ex)AmplitudeilmaisimetkallioperäSpeed of soundNeutrinoAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)Order of magnitudeEnergy (signal processing)Geology
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Influence of pre-existing microstructure on mechanical properties of marine ice during compression experiments

2014

AbstractMarine ice is an important component of ice shelves in Antarctica. It accretes in substantial amounts at weak points and below ice shelves. It is likely to exhibit peculiar rheological properties, which are crucial to understanding its potential role in stabilizing ice-shelf flow. Due to its location and consolidation processes, marine ice can present a variety of textures which are likely to influence its rheological properties. We present a new dataset of unconfined uniaxial compression experiments on folded marine ice samples that have been cut at various angles to the folds. Texture and fabric analyses are described ‘before’ and ‘after’ the deformation experiment. It is shown th…

geographygeography.geographical_feature_category010504 meteorology & atmospheric sciencesConsolidation (soil)MineralogyPressure ridge010502 geochemistry & geophysics01 natural sciencesIce shelfPhysics::GeophysicsCreepSea ice growth processesRheologyPerpendicularGeotechnical engineeringAstrophysics::Earth and Planetary AstrophysicsAnisotropyPhysics::Atmospheric and Oceanic PhysicsGeology0105 earth and related environmental sciencesEarth-Surface ProcessesJournal of Glaciology
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Net radiation of the Iberian Peninsula from NOAA-AVHRR data

1998

In this work, we present a methodology to obtain the daily net radiation flux from NOAA-AVHRR data. To get this objective we need firstly to obtain shortwave net radiation flux from the solar global radiation flux and the albedo map. Secondly, we need to obtain the upward longwave radiation flux from surface temperature and emissivity and the downward longwave radiation flux from air temperature. Like an example of application of this methodology a daily net radiation flux image of the Iberian Peninsula is presented, in which we show that daily net radiation flux can be obtained with a satisfactory precision lower than 1.0 mmday -1 .

geographygeography.geographical_feature_categoryAstrophysics::High Energy Astrophysical PhenomenaFluxRadiationAtmospheric sciencesRadiation fluxNet radiometerPeninsulaClimatologyNet radiationEmissivityEnvironmental scienceShortwavePhysics::Atmospheric and Oceanic PhysicsSPIE Proceedings
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Relationships between diffuse CO 2 emissions and volcanic activity on the island of Vulcano (Aeolian Islands, Italy) during the period 1984-1994

2002

Measurements of CO2 flux from the ground were periodically carried out on the island of Vulcano (Aeolian Islands, Italy) between 1984 and 1994. Three high-flux areas were identified at the foot of the volcanic cone (La Fossa), either inside or very close to the main village. Effect of the choice of the sampling grid was evaluated. A different sampling grid resulted in similar distribution patterns, but with different CO2 fluxes. Therefore, the absolute estimate of the total flux from the investigated area includes a large degree of uncertainty, but repeated measurements with permanent sampling sites are accurate and can detect small changes. No correlation of the flux with atmospheric param…

geographygeography.geographical_feature_categoryAstrophysics::High Energy Astrophysical PhenomenaSoil gasMineralogySampling (statistics)Atmospheric sciencesFumarolePhysics::GeophysicsMediterranean seaFlux (metallurgy)VolcanoGeochemistry and PetrologyAeolian processesVolcanic conePhysics::Atmospheric and Oceanic PhysicsGeologyBulletin of Volcanology
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Esa's SMOS Mission – Supporting Agricultural Applications

2018

The European Space Agency's (ESA) SMOS mission, in orbit since more than 8 years, carries a passive microwave interferometric radiometer measuring in L-Band and provides accurate global observations of emitted radiation originating from the Earth's surfaces since the atmosphere is almost transparent in this spectral range. In addition, over land the effect of vegetation on the measurements is smaller than for shorter wavelengths. The scientific objectives of the SMOS mission directly respond to the need for global observations of soil moisture and ocean salinity, two key variables used in predictive hydrological, oceanographic and atmospheric models. SMOS observations also provide informati…

geographygeography.geographical_feature_categoryAtmospheric modelsVegetationSnowPhysics::GeophysicsAtmosphereBrightness temperatureOrbit (dynamics)Sea iceEnvironmental scienceAstrophysics::Earth and Planetary AstrophysicsPhysics::Atmospheric and Oceanic PhysicsInterferometric radiometerRemote sensingIGARSS 2018 - 2018 IEEE International Geoscience and Remote Sensing Symposium
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Spectroscopic capture of 1 Hz volcanic SO2fluxes and integration with volcano geophysical data

2009

[1] Here we present a novel spectroscopic approach to capturing, with unprecedented time resolution and accuracy, volcanic SO2 fluxes. This is based on two USB2000 spectrometers, coupled to cylindrical lens telescopes, each collecting light which has transited horizontal sections of the rising plume. We report on field data from Stromboli volcano, in which the entire emission rate from the volcano was measured, as well as flux signatures associated with individual crater explosions. The latter were integrated with seismic and thermal data, demonstrating correlations in both cases, and representing the first such geophysical-geochemical data corroboration on this timescale. Such a holistic e…

geographygeography.geographical_feature_categoryExplosive materialSpectrometerAstrophysics::High Energy Astrophysical Phenomenavolcanic degassing doas so2GeophysicsPhysics::GeophysicsPlumeGeophysicsImpact craterVolcanoThermalPanacheGeneral Earth and Planetary SciencesAstrophysics::Earth and Planetary AstrophysicsCylindrical lensPhysics::Atmospheric and Oceanic PhysicsSeismologyGeologyGeophysical Research Letters
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Experimental deformation of deuterated ice in 3D and 2D: identification of grain-scale processes

2015

Major polar ice sheets and ice caps experience cycles of variable flow during different glacial periods and as a response to past warming. The rate and localisation of deformation inside an ice body controls the evolution of ice microstructure and crystallographic fabric. This is critical for interpreting proxy signals for climate change, with deformation overprinting and disrupting stratigraphy deep under ice caps due to the nature of the flow. The final crystallographic fabric in polar ice sheets provides a record of deformation history, which in turn controls the flow properties of ice during further deformation and affects geophysical sensing of ice sheets. For example, identification o…

geography.geographical_feature_categoryEcologyMeteorologyClimate changeGeologyGeophysicsGrain sizeProxy (climate)Physics::GeophysicsIce-sheet modelGeographyAstrophysics::Earth and Planetary AstrophysicsGlacial periodClimate stateLayeringIce sheetPhysics::Atmospheric and Oceanic PhysicsProceedings of the Royal Society of Victoria
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