Search results for " objects"

showing 10 items of 186 documents

Discovery of off-axis jet structure of TeV blazar Mrk 501 with mm-VLBI

2016

Context. High-resolution millimeter wave very-long-baseline interferometry (mm-VLBI) is an ideal tool for probing the structure at the base of extragalactic jets in detail. The TeV blazar Mrk 501 is one of the best targets among BL Lac objects for studying the nature of off-axis jet structures because it shows different jet position angles at different scales. Aims. The aim of this study is to investigate the properties of the off-axis jet structure through high-resolution mm-VLBI images at the jet base and physical parameters such as kinematics, flux densities, and spectral indices. Methods. We performed Very Long Baseline Array (VLBA) observations over six epochs from 2012 February to 201…

Astrofísicaactive [Galaxies]010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxContext (language use)galaxies [Radio continuum]Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesRadio continuum: galaxiesindividual: Markarian 501 [BL Lacertae objects]0103 physical sciencesVery-long-baseline interferometryBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsVery Long Baseline Array0105 earth and related environmental sciencesHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Spectral indexBL Lacertae objects: individual: Markarian 501 galaxies: active galaxies: jets radio continuum: galaxiesAstrophysics::Instrumentation and Methods for AstrophysicsAstronomy and AstrophysicsGalaxies: activeAstrophysics - Astrophysics of GalaxiesBL Lacertae objects: individual: Markarian 501Galaxies: jetsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astronomiajets [Galaxies]MillimeterAstrophysics - High Energy Astrophysical PhenomenaAstronomy & Astrophysics
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Thermal emission, shock modification, and X-ray emitting ejecta in SN 1006

2009

Efficient particle acceleration can modify the structure of supernova remnants. In this context we present the results of the combined analysis of the XMM-Newton EPIC archive observations of SN 1006. We aim at describing the spatial distribution of the physical and chemical properties of the X-ray emitting plasma at the shock front. We investigate the contribution of thermal and non-thermal emission to the X-ray spectrum at the rim of the remnant to study how the acceleration processes affect the X-ray emitting plasma. We perform a spatially resolved spectral analysis on a set of regions covering the whole rim of the shell and we exploit the results of the spectral analysis to produce a cou…

Astrophysics::High Energy Astrophysical PhenomenaCiencias FísicasFOS: Physical sciencesContext (language use)AstrophysicsISM: individual objects: SN 1006ISM [X-RAYS]//purl.org/becyt/ford/1 [https]ThermalSUPERNOVA REMNANTS [ISM]EjectaISM: supernova remnantAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstronomy and AstrophysicsPlasma//purl.org/becyt/ford/1.3 [https]X-rays: ISMShock (mechanics)Particle accelerationAstronomíaSupernovaINDIVIDUAL OBJECTS: SN 1006 [ISM]Space and Planetary ScienceMagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTAS
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X-ray emitting structures in the Vela SNR: ejecta anisotropies and progenitor stellar wind residuals

2021

The Vela supernova remnant (SNR) shows several ejecta fragments protruding beyond the forward shock (shrapnel). Recent studies have revealed high Si abundance in two shrapnel (A and G), located in opposite directions with respect to the SNR center. This suggests the possible existence of a Si-rich jet-counterjet structure. We analyzed an XMM-Newton observation of a bright clump, behind shrapnel G, which lies along the direction connecting A and G. The aim is to study the physical and chemical properties of this clump to ascertain whether it is part of this putative jet-like structure. We produced background-corrected and adaptively-smoothed count-rate images and median photon energy maps, a…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)AstrophysicsISM [X-RAYS]Photon energyVela01 natural sciences//purl.org/becyt/ford/1 [https]Protein filamentSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesROSATAstrophysics::Solar and Stellar AstrophysicsSUPERNOVA REMNANTS [ISM]Ejecta010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsISM: supernova remnantsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsVela Supernova Remnant010308 nuclear & particles physicsAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]X-rays: ISMSupernovaISM: individual objects: Vela SNRSpace and Planetary ScienceINDIVIDUAL OBJECTS: VELA SNR [ISM]Astrophysics - High Energy Astrophysical PhenomenaAstronomy & Astrophysics
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Gamma-Ray Flares from Mrk421 in 2008 observed with the ARGO-YBJ detector

2010

In 2008 the blazar Markarian 421 entered a very active phase and was one of the brightest sources in the sky at TeV energies, showing frequent flaring episodes. Using the data of ARGO-YBJ, a full coverage air shower detector located at Yangbajing (4300 m a.s.l., Tibet, China), we monitored the source at gamma ray energies E > 0.3 TeV during the whole year. The observed flux was variable, with the strongest flares in March and June, in correlation with X-ray enhanced activity. While during specific episodes the TeV flux could be several times larger than the Crab Nebula one, the average emission from day 41 to 180 was almost twice the Crab level, with an integral flux of (3.6 +-0.6) 10^-1…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesFluxAstrophysicsBL Lacertae objectSettore FIS/05 - Astronomia E AstrofisicaExtended Air showersSettore FIS/05 - Astronomia e Astrofisicageneral" ["gamma rays]BlazarBL Lacertae objects; Markarian 421; gamma rays; Extended Air showersCherenkov radiationHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsSpectral indexindividual (Markarian 421)" ["BL Lacertae objects]Markarian 421Settore FIS/01 - Fisica SperimentaleGamma rayindividual (Markarian 421) - gamma rays: observations [BL Lacertae objects]Astronomy and AstrophysicsAir showerCrab NebulaSpace and Planetary Sciencegamma rayIntergalactic travelAstrophysics - High Energy Astrophysical Phenomena
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The shape of the cutoff in the synchrotron emission of SN 1006 observed with XMM-Newton

2013

Synchrotron X-ray emission from the rims of young supernova remnants allows us to study the high-energy tail of the electrons accelerated at the shock front. The analysis of X-ray spectra can provide information on the physical mechanisms that limit the energy achieved by the electrons in the acceleration process. We aim at verifying whether the maximum electron energy in SN 1006 is limited by synchrotron losses and at obtaining information on the shape of the cutoff in the X-ray synchrotron emission. We analyzed the deep observations of the XMM-Newton SN 1006 Large Program. We performed spatially resolved spectral analysis of a set of small regions in the nonthermal limbs and studied the X…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesISM: individual objects: SN 1006AstrophysicsElectron01 natural sciencesSpectral linelaw.inventionMomentumAccelerationlaw0103 physical sciencesRadiative transferCutoff010306 general physics010303 astronomy & astrophysicsISM: supernova remnantAstrophysics::Galaxy AstrophysicsISM: supernova remnantsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAstronomy and AstrophysicsAstronomy and AstrophysicX-rays: ISMSynchrotronSupernovaSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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The Petite Seine in the metal Ages, an obligatory route on the Tin Road

2021

AubeTin RoadBurgundy sill[SHS.ARCHEO] Humanities and Social Sciences/Archaeology and PrehistorySeine basintrade controlSaône valleyenclosed burial sitesdeposits of metal objectshilltop sites[SHS.ARCHI] Humanities and Social Sciences/Architecture space managementYonne
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The NHXM observatory

2011

Exploration of the X-ray sky has established X-ray astronomy as a fundamental astrophysical discipline. While our knowledge of the sky below 10 keV has increased dramatically (∼8 orders of magnitude) by use of grazing incidence optics, we still await a similar improvement above 10 keV, where to date only collimated instruments have been used. Also ripe for exploration is the field of X-ray polarimetry, an unused fundamental tool to understand the physics and morphology of X-ray sources. Here we present a novel mission, the New Hard X-ray Mission (NHXM) that brings together for the first time simultaneous high-sensitivity, hard-X-ray imaging, broadband spectroscopy and polarimetry. NHXM will…

Black-holesAcceleration mechanismCosmic Visionmedia_common.quotation_subjectPolarimetry7. Clean energy01 natural sciencesMissionsCosmologyPhysical cosmologyNon-thermal emissionAcceleration mechanism; Accretion physics; Black-holes; Compact objects; Cosmology; Missions; Non-thermal emission; X-ray imaging; X-ray polarimetry; Astronomy and Astrophysics; Space and Planetary ScienceObservatory0103 physical sciencesBroadbandX-ray polarimetry010303 astronomy & astrophysicsCompact objectsmedia_commonPhysics010308 nuclear & particles physicsX-ray imagingVegaAstronomyAstronomy and AstrophysicsAccretion physicsCosmologySkySpace and Planetary ScienceExperimental Astronomy
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Relativistic beaming and gamma-ray brightness of blazars

2009

We investigate the dependence of gamma-ray brightness of blazars on intrinsic properties of their parsec-scale radio jets and the implication for relativistic beaming. By combining apparent jet speeds derived from high-resolution VLBA images from the MOJAVE program with millimetre-wavelength flux density monitoring data from Metsahovi Radio Observatory, we estimate the jet Doppler factors, Lorentz factors, and viewing angles for a sample of 62 blazars. We study the trends in these quantities between the sources which were detected in gamma-rays by the Fermi Large Area Telescope (LAT) during its first three months of science operations and those which were not detected. The LAT-detected blaz…

BrightnessCosmology and Nongalactic Astrophysics (astro-ph.CO)Astrophysics::High Energy Astrophysical Phenomenajets [galaxies]FOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionTelescopesymbols.namesakeRelativistic beaminglawquasars: general0103 physical sciencesBlazar010303 astronomy & astrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::GalaxiasHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsgeneral [quasars]general [BL Lacertae objects]010308 nuclear & particles physicsGamma rayAstronomy and Astrophysicsgalaxies: jetsViewing angle:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Galaxias [UNESCO]Lorentz factorSpace and Planetary Scienceactive [galaxies]BL Lacertae objectssymbolsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaAstrophysics - High Energy Astrophysical Phenomenagalaxies: active; ; ; BL Lacertae objects : generalFermi Gamma-ray Space TelescopeAstrophysics - Cosmology and Nongalactic Astrophysics
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Domain-Specific Characteristics of Data Quality

2017

The research discusses the issue how to describe data quality and what should be taken into account when developing an universal data quality management solution. The proposed approach is to create quality specifications for each kind of data objects and to make them executable. The specification can be executed step-by-step according to business process descriptions, ensuring the gradual accumulation of data in the database and data quality checking according to the specific use case. The described approach can be applied to check the completeness, accuracy, timeliness and consistency of accumulated data.

Business processComputer sciencecomputer.file_formatcomputer.software_genreElectronic mailData modelingUnified Modeling LanguageData qualityData miningExecutableCompleteness (statistics)Data objectscomputercomputer.programming_languageProceedings of the 2017 Federated Conference on Computer Science and Information Systems
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A Metaphor for Identities in Transition through Urbanization and Globalization: Tofu and One Hundred Surnames

2019

The Chinese artist Chen Qiulin has been taking displacement and the resulting unrest in people’s identity as her persistent theme since the early 1990s. Focusing on a series of her works made since 2004 dealing explicitly with tofu and Chinese surnames, this paper examines her exploration of identities in transition in the context of China’s mass urbanization and globalization. By showing the artist’s conceptual evolution, her preference for materials and mediums, and her exhibition strategy, this paper explores two issues. First, it illuminates how the artist has transformed “tofu” and “surname” into a metaphor for the dilemma of identity under the urbanization in China. Second, it discuss…

ChinaCultural identityMetaphormedia_common.quotation_subjectIdentity (social science)Context (language use)diasporacontemporary artDiasporaContemporary artGlobalizationnykytaideta616identiteettiSociologyChinalcsh:History of the artsmedia_commonmuisti (kognitio)urbanisationta6132memory (cognition)AestheticsKiinakaupungistuminenArtikkelitlcsh:NX440-632identity (mental objects)Tahiti
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