Search results for "OBJECTS"

showing 10 items of 197 documents

Gaia-ESO Survey: Gas dynamics in the Carina nebula through optical emission lines

2016

Aims. We present observations from the Gaia-ESO Survey in the lines of Hα, [N II], [S II], and He I of nebular emission in the central part of the Carina nebula. Methods. We investigate the properties of the two already known kinematic components (approaching and receding), which account for the bulk of emission. Moreover, we investigate the features of the much less known low-intensity high-velocity (absolute RV >50 km s) gas emission. Results. We show that gas giving rise to Hα and He I emission is dynamically well correlated with but not identical to gas seen through forbidden-line emission. Gas temperatures are derived from line-width ratios, and densities from [S II] doublet ratios. Th…

HII regionsastro-ph.SRastro-ph.GAAstrophysics::High Energy Astrophysical PhenomenaShell (structure)FluxFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesISM: individual objects: Carina nebula; ISM: general ; HII regionsIonization0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsHII regionEmission spectrum010303 astronomy & astrophysicsISM: individual objects: Carina nebulaQCSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsQBISM: generalAstronomía y AstrofísicaPhysicsNebulageneral [ISM]010308 nuclear & particles physicsindividual objects: Carina nebula [ISM]Astronomy and AstrophysicsGas dynamicsAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesDust laneCore (optical fiber)Astrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)HII regions; ISM: general; ISM: individual objects: Carina nebula; Astronomy and Astrophysics; Space and Planetary Science
researchProduct

A search for anisotropy in the arrival directions of ultra high energy cosmic rays recorded at the Pierre Auger Observatory

2012

Observations of cosmic ray arrival directions made with the Pierre Auger Observatory have previously provided evidence of anisotropy at the 99% CL using the correlation of ultra high energy cosmic rays (UHECRs) with objects drawn from the Véron-Cetty Véron catalog. In this paper we report on the use of three catalog independent methods to search for anisotropy. The 2pt–L, 2pt+ and 3pt methods, each giving a different measure of selfclustering in arrival directions, were tested on mock cosmic ray data sets to study the impacts of sample size and magnetic smearing on their results, accounting for both angular and energy resolutions. If the sources of UHECRs follow the same large scale structu…

HIRES STEREO[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomySMALL-SCALE ANISOTROPYAstrophysics01 natural sciencesAltas energíasCosmic Rays ShowerCosmologyUltra-high-energy cosmic rayAnisotropy010303 astronomy & astrophysicsmedia_commonPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)[PHYS]Physics [physics]BL-LACERTAEAstrophysics::Instrumentation and Methods for AstrophysicsPierre Auger ObservatoryRadiación cósmicaFísica nuclearOBJECTSAstrophysics - High Energy Astrophysical Phenomenacosmic ray experiments; ultra high energy cosmic raysACTIVE GALACTIC NUCLEIActive galactic nucleusmedia_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCosmic raysearch for anisotropyultra high energy cosmic raysCosmic Ray[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciences010306 general physicsCiencias ExactasPierre Auger ObservatorySPECTRUMAstronomyFísicaAstronomy and AstrophysicsASTROFÍSICAUniverseGalaxyExperimental High Energy Physicsanisotrpycosmic ray experiments[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]cosmologyJournal of Cosmology and Astroparticle Physics
researchProduct

The origin of the X-ray-emitting plasma in the eastern edge of the Cygnus Loop

2010

The Cygnus Loop is interacting with a protrusion of the cavity wall in its eastern edge (the XA region), where the X-ray emission is very bright. The complexity of the environment and the non-linear physical processes of the shock-cloud interaction make the origin of the X-ray emission still not well understood. Our purpose is to understand the physical origin of the X-ray emission in the XA region, addressing, in particular, the role of thermal conduction in the interaction process. We analyzed two XMM-Newton data sets, performing image analysis and spatially resolved spectral analysis on a set of homogeneous regions. We applied a recently developed diagnostic tool to compare spectral anal…

High Energy Astrophysical Phenomena (astro-ph.HE)ISM: cloudAstrophysics::High Energy Astrophysical PhenomenaISM: individual objects: G74.0-8.5FOS: Physical sciencesAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy AstrophysicsISM: supernova remnantX-rays: ISMISM: individual objects: Cygnus Loop
researchProduct

Unveiling the spatial structure of the overionized plasma in the supernova remnant W49B

2011

W49B is a mixed-morphology supernova remnant with thermal X-ray emission dominated by the ejecta. In this remnant, the presence of overionized plasma has been directly established, with information about its spatial structure. However, the physical origin of the overionized plasma in W49B has not yet been understood. We investigate this intriguing issue through a 2D hydrodynamic model that takes into account, for the first time, the mixing of ejecta with the inhomogeneous circumstellar and interstellar medium, the thermal conduction, the radiative losses from optically thin plasma, and the deviations from equilibrium of ionization induced by plasma dynamics. The model was set up on the basi…

High Energy Astrophysical Phenomena (astro-ph.HE)ISM: individual objects: W49BPhysics::Plasma PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics - High Energy Astrophysical PhenomenaISM: individual objects: G43.3-0.2Astrophysics::Galaxy Astrophysicshydrodynamicmethods: numericalISM: supernova remnants
researchProduct

Unveiling pure-metal ejecta X-ray emission in supernova remnants through their radiative recombination continuum

2020

Spectral analysis of X-ray emission from ejecta in supernova remnants (SNRs) is hampered by the low spectral resolution of CCD cameras, which creates a degeneracy between the best-fit values of abundances and emission measure. The combined contribution of shocked ambient medium and ejecta to the X-ray emission complicates the determination of the ejecta mass and chemical composition, leading to big uncertainties in mass estimates and it can introduce a bias in the comparison between the observed ejecta composition and the yields predicted by explosive nucleosynthesis. We explore the capabilities of present and future spectral instruments with the aim of identifying a spectral feature which …

High Energy Astrophysical Phenomena (astro-ph.HE)Physics010504 meteorology & atmospheric sciencesSpectrometerAstrophysics::High Energy Astrophysical PhenomenaBremsstrahlungFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics01 natural sciencesSpectral lineSupernovaSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceNucleosynthesis0103 physical sciencesISM: abundances ISM: individual objects: Cas A ISM: supernova remnants X-rays: general X-rays: individuals: Cas AAstrophysics::Solar and Stellar AstrophysicsSpontaneous emissionSpectral resolutionAstrophysics - High Energy Astrophysical PhenomenaEjecta010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciences
researchProduct

Spatial distribution of X-ray emitting ejecta in Tychos SNR: indications of shocked Titanium

2015

Young supernova remnants show a characteristic ejecta-dominated X-ray emission that allows us to probe the products of the explosive nucleosynthesis processes and to ascertain important information about the physics of the supernova explosions. Hard X-ray observations have recently revealed the radioactive decay lines of 44Ti at ~67.9 keV and ~78.4 keV in the Tycho's SNR. We here analyze the set of XMM-Newton archive observations of the Tycho's SNR. We produce equivalent width maps of the Fe K and Ca XIX emission lines and find indications for a stratification of the abundances of these elements and significant anisotropies. We then perform a spatially resolved spectral analysis by identify…

High Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSpectral lineISM: individual objects: Tycho's SNR ISM: supernova remnants X-rays: ISMSupernovaSpace and Planetary ScienceNucleosynthesisAstrophysics::Solar and Stellar AstrophysicsEmission spectrumAstrophysics - High Energy Astrophysical PhenomenaEjectaAnisotropyEquivalent widthRadioactive decayAstrophysics::Galaxy Astrophysics
researchProduct

Born–Infeld inspired modifications of gravity

2017

General Relativity has shown an outstanding observational success in the scales where it has been directly tested. However, modifications have been intensively explored in the regimes where it seems either incomplete or signals its own limit of validity. In particular, the breakdown of unitarity near the Planck scale strongly suggests that General Relativity needs to be modified at high energies and quantum gravity effects are expected to be important. This is related to the existence of spacetime singularities when the solutions of General Relativity are extrapolated to regimes where curvatures are large. In this sense, Born-Infeld inspired modifications of gravity have shown an extraordin…

High Energy Physics - Theorystar: compactcosmological model[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]space-time: black holeGeneral Physics and AstronomyAstrophysics01 natural sciencesGeneral Relativity and Quantum Cosmology[ PHYS.HTHE ] Physics [physics]/High Energy Physics - Theory [hep-th]Gravitationquantum gravity: effectBorn–Infeld gravityPhysicsenergy: highBlack holes[PHYS.HTHE]Physics [physics]/High Energy Physics - Theory [hep-th]formationCosmologyregularizationcurvaturewormhole[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Gravitational singularitySingularitiesAstrophysics - Cosmology and Nongalactic AstrophysicsGravity (chemistry)Cosmology and Nongalactic Astrophysics (astro-ph.CO)General relativityEarly universegeneral relativity: solutionFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]Theoretical physicsGeneral Relativity and Quantum Cosmologyspace-time: singularity0103 physical sciencesunitaritystructureWormholeinflation010306 general physicsCompact objectsSpacetime010308 nuclear & particles physicsscale: PlanckBlack holeBorn-Infeld modelHigh Energy Physics - Theory (hep-th)gravitationQuantum gravity[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
researchProduct

Highlights from the ARGO-YBJ Experiment

2012

""The ARGO-YBJ experiment at YangBaJing in Tibet (4300m a.s.l.) has been taking data with its full layout since October 2007. Here we present a few significant results obtained in gamma-ray astronomy and cosmic-ray physics. Emphasis is placed on the analysis of gamma-ray emission from point-like sources (Crab Nebula, MRK 421), on the preliminary limit on the antiproton\\\/proton flux ratio, on the large-scale cosmic-ray anisotropy and on the proton-air cross-section. The performance of the detector is also discussed, and the perspectives of the experiment are outlined.""

HistoryAstronomyFluxAstrophysicsProton flux01 natural sciencesArgo-YbjGamma-ray emissionSettore FIS/05 - Astronomia E AstrofisicaCosmic-ray physicsResistive Plate ChambersInstrumentation010303 astronomy & astrophysicsArgoPhysicsRange (particle radiation)DetectorSettore FIS/01 - Fisica SperimentaleCrab nebulaAstrophysics::Instrumentation and Methods for AstrophysicsGamma rayCrab nebula Extensive air showers Flux ratio Gamma-ray astronomy Gamma-ray emission Ground based Resistive plate chambers; Astronomy Cosmic rays Cosmology Experiments; Gamma raysFlux ratioCosmologyComputer Science ApplicationsResistive plate chambersNuclear and High Energy PhysicsX- and γ-ray instrumentGround-based gamma-ray astronomyAstrophysics::High Energy Astrophysical PhenomenaExtensive air showerCosmic rayAstrophysics::Cosmology and Extragalactic AstrophysicsCosmic RayEducationResistive Plate Chambers Extensive air showers Ground-based g ray astronomy Cosmic-ray physicsGround-based γ-ray astronomy0103 physical sciencesExtensive air showersCosmic raysExtensive air showers X- and γ-ray instruments Pulsars. Quasars active or peculiar galaxies objects and systemsAstrophysics::Galaxy AstrophysicsGamma-ray astronomy010308 nuclear & particles physicsGamma raysAstronomyResistive Plate ChamberGround basedCrab NebulaAntiprotonResistive Plate Chambers; Extensive air showers; Ground-based γ-ray astronomy; Cosmic-ray physicsSatelliteGamma-ray burstExperimentsJournal of Physics: Conference Series
researchProduct

Curating Objects from the European Border Zone: The “Lampedusa Refugee Boat”

2019

The cultural politics of the present encourage museums and artists to seek an ethical vision within Europe navigating the knowledge of ongoing mass death at the border. This is one explanation for the interest in objects symbolising present-day irregular border crossing among museum curators, artists, designers and activists. Wooden fishing boats, inflatable dinghies and life jackets appear regularly in exhibitions and installations. This chapter focuses on the meaning of “the Lampedusa boat” and argues that the narrative context within which the boats are exhibited guides the work of imagination that animates the object. While exhibiting the boats carries the critical potential to relocate…

HistorybiologyRefugeemuistin politiikkarajatContext (language use)kuolemabiology.organism_classificationObject (philosophy)objectsborder deathspakolaisuusVisual artsExhibitionPoliticsNarrativemuseumsmuseoesineetLampedusaartMeaning (linguistics)
researchProduct

Print and online newspapers as material artefacts

2014

Traditional newspaper journalism is in a state of crisis and there have been several attempts to overcome this. Many discourses have reiterated the triumphal march of a digital revolution in newspaper journalism and anticipated the end of the print newspaper. This moment calls for an in-depth analysis of reader habits of news consumption and use in order to understand the audiences for journalistic output and their relationship with the journalistic objects. In this study, we adopt a multi-method approach, integrating (1) qualitative content analysis of student essays dealing with the physicality of printed and online newspapers, (2) ethnographic observation of the use practices of readers…

Historymedia_common.quotation_subjectritualizationemotioncomputer.software_genrereadershipNewspaperprint newspaperArts and Humanities (miscellaneous)State (polity)eleetonline newspaperRitualizationta518use practicesmedia_commonMultimediaCommunicationgesturesMedia studiesta5142posturesAudience measurementComputingMethodologies_DOCUMENTANDTEXTPROCESSINGJournalismEmotion; gestures; material objects; online newspaper; postures; print newspaper; readership; ritualization; use practicesDigital Revolutioncomputermaterial objectsGestureJournalism
researchProduct