Search results for "Inari"

showing 10 items of 735 documents

INTEGRAL observations of the peculiar BeX System SAX J2103.5+4545

2004

We present an INTEGRAL data analysis of the X-ray transient \object{SAX J2103.5+4545} during two outbursts detected in December 2002. The INTEGRAL coordinates and error circle agree with the position of the recently proposed optical counterpart. A power-law plus cut-off model provided a good fit to the 4-150 keV spectrum yielding a photon index of 1.0+-0.1, a cut-off energy E_cut=7.6+-2.0 keV and a folding energy E_fold=30.9+-2.5 keV. The X-ray luminosity in the 4-150 keV energy range was found to be 6.0x10^36 erg/s, assuming a distance of 6.5 kpc. This luminosity, together with the derived photon index, indicate that the source is in a bright state. A 354.9$+-0.5 second pulse period is mea…

AccretionPhotonAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesValue (computer science)AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsLuminosityPulse periodPosition (vector)X-raysBright statePhysicsRange (particle radiation)Astrophysics (astro-ph)BinariesSAX J2103.5+4545 [Pulsars]BeAstronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Space and Planetary ScienceAccretion disksUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaEmission-lineAccretion ; Accretion disks ; Binaries ; Emission-line ; Be ; Pulsars : SAX J2103.5+4545 ; X-rays ; Binaries:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Energy (signal processing)Astronomy & Astrophysics
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Broadband X-ray spectral variability of the pulsing ULX NGC 1313 X-2

2021

[Context] It is thought that ultraluminous X-ray sources (ULXs) are mainly powered by super-Eddington accreting neutron stars or black holes as shown by the recent discovery of X-ray pulsations and relativistic winds. [Aims] This work presents a follow-up study of the spectral evolution over two decades of the pulsing ULX NGC 1313 X-2 in order to understand the structure of the accretion disc. The primary objective is to determine the shape and nature of the dominant spectral components by investigating their variability with the changes in the source luminosity. [Methods[ We performed a spectral analysis over the canonical 0.3-10.0 keV energy band of all the high signal-to-noise XMM-Newton…

AccretionULXsAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)Astrophysicsindividuals: NGC 1313 X-2 [X-rays]Astrophysics::Cosmology and Extragalactic AstrophysicsSpectral lineSettore FIS/05 - Astronomia E AstrofisicaX-rays: Individuals: NGC 1313 X-2ThermalCutoffAstrophysics::Solar and Stellar AstrophysicsBlack-body radiationX-rays: BinariesAstrophysics::Galaxy AstrophysicsPhysicsastro-ph.HEHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)Astronomy and AstrophysicsRadiusAccretion accretion disksNeutron starSpace and Planetary ScienceAccretion disksbinaries [X-rays]Astrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaX-rays: individuals:NGC 1313 X-2
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IGR J17503–2636: a candidate supergiant fast X-ray transient

2019

IGR J17503-2636 is a hard X-ray transient discovered by INTEGRAL on 2018 August 11. This was the first ever reported X-ray emission from this source. Following the discovery, follow-up observations were carried out with Swift, Chandra, NICER, and NuSTAR. We report in this paper the analysis and results obtained from all these X-ray data. Based on the fast variability in the X-ray domain, the spectral energy distribution in the 0.5-80 keV energy range, and the reported association with a highly reddened OB supergiant at ~10 kpc, we conclude that IGR J17503-2636 is most likely a relatively faint new member of the supergiant fast X-ray transients. Spectral analysis of the NuSTAR data revealed …

AccretionX-ray transientAstrophysics::High Energy Astrophysical PhenomenaCyclotronFOS: Physical sciencesAstrophysics01 natural scienceslaw.inventionbinaries [x-rays]X-rays: binariesSettore FIS/05 - Astronomia E AstrofisicaMethods: observationalBinaries: closelaw0103 physical sciencesSpectral analysis010303 astronomy & astrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)individuals: IGR J17503-2636 [X-rays]010308 nuclear & particles physicsScatteringAstronomy and AstrophysicsStars: neutronAccretion (astrophysics)Neutron starAccretion diskSpace and Planetary ScienceSpectral energy distributionSupergiantAstrophysics - High Energy Astrophysical PhenomenaAstronomy & Astrophysics
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Aperiodic variability of low-mass X-ray binaries at very low frequencies

2003

We have obtained discrete Fourier power spectra of a sample of persistent low-mass neutron-star X-ray binaries using long-term light curves from the All Sky Monitor on board the Rossi X-ray Timing Explorer. Our aim is to investigate their aperiodic variability at frequencies in the range 1 x 10^{-7}-5 x 10^{-6} Hz and compare their properties with those of the black-hole source Cyg X-1. We find that the classification scheme that divides LMXBs into Z and atoll sources blurs at very low frequencies. Based on the long-term (~ years) pattern of variability and the results of power-law fits (P ~ v^{-a}) to the 1 x 10^{-7}-5 x 10^{-6} Hz power density spectra, low-mass neutron-star binaries fall…

Accretionmedia_common.quotation_subjectFOS: Physical sciencesAstrophysicsNeutronAstrophysicsNeutron ; Binaries ; X-rays ; Binaries ; Accretion ; Accretion discsUNESCO::ASTRONOMÍA Y ASTROFÍSICASpectral lineX-raysNeutronmedia_commonPhysicsAccretion (meteorology)Astrophysics (astro-ph)BinariesX-rayAstronomy and AstrophysicsLight curve:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Space and Planetary ScienceAperiodic graphSkyUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaLow MassAccretion discs:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Accrétion et éjection dans les systèmes binaires X transitoires à trous noirs : le cas de GRS 1716-249

2020

I buchi neri transienti (BHT) sono tra le sorgenti con emissione ai raggi X più luminose della galassia. Grazie all’elevato flusso in banda X e alla loro alta variabilità temporale. queste sorgenti offrono un’opportunità unica per studiare la fisica dell’accrescimento in straordinareie condizioni fisiche. I BHT mostrano episodici outburst caratterizzati da diverse luminosità in banda X e γ, diverse forme spettrali e proprietà della variabilità temporale. L’obiettivo di questa tesi è lo studio della geometria, dei meccanismi e dei processi fisici coinvolti nell’emissione del buco nero transiente GRS 716-249. Di seguito presento l’analisi spettrale e temporale delle osservazioni della GRS 171…

AccrétionTrou noir physiqueAccretionX-rays : binaries[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Gamma-rays : generalRayons X : binairesgamma-rays: generalBlack hole physicsDisque d'accrétionX-rays: generalRayons X : généralstars: jetsX-rays: binariesSettore FIS/05 - Astronomia E Astrofisicaaccretion accretion discsÉtoiles : jetRayons gamma : généralStars : jetsAccretion discsX-rays : general
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Dissipative Processes and Their Role in the Evolution of Radio Galaxies

2019

Particle acceleration in relativistic jets to very high energies occurs at the expense of the dissipation of magnetic or kinetic energy. Therefore, understanding the processes that can trigger this dissipation is key to the characterization of the energy budgets and particle acceleration mechanisms at action in active galaxies. Instabilities and entrainment are two obvious candidates to trigger dissipation. On the one hand, supersonic, relativistic flows threaded by helical fields, as expected from the standard formation models of jets in supermassive black-holes, are unstable to a series of magnetohydrodynamical instabilities, such as the Kelvin-Helmholtz, current-driven, or possibly the p…

Active galactic nucleuslcsh:AstronomyRadio galaxyAstrophysics::High Energy Astrophysical Phenomenagalaxies: activeFOS: Physical sciencesKinetic energy01 natural scienceslcsh:QB1-991X-rays: binariesAstrophysical jet0103 physical sciencesrelativistic processes ISM: jets and outflows010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)010308 nuclear & particles physicsAstronomy and AstrophysicsMechanicsgalaxies: jetsradiation mechanisms: non-thermalDissipationAstrophysics - Astrophysics of GalaxiesParticle accelerationAstrophysics of Galaxies (astro-ph.GA)MagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenamagnetohydrodynamicsGalaxies
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Enhanced oxidative susceptibility and reduced antioxidant content of metabolic precursors of small, dense low-density lipoproteins.

2001

Abstract PURPOSE: Elevated plasma concentrations of low-density lipoproteins (LDL) increase risk for coronary heart disease. However, lipoprotein profiles rich in small, dense LDL particles confer greater risk than those that mainly consist of large, buoyant LDL. This may be due, in part, to the greater oxidative susceptibility of small, dense LDL. In the current studies, we tested whether differences in the oxidative behavior of buoyant and dense LDL arise from differences in their immediate metabolic precursors, intermediate-density lipoproteins. SUBJECTS AND METHODS: We compared the properties of intermediate-density lipoproteins and buoyant and dense LDL subfractions in 9 subjects with …

AdultMalemedicine.medical_specialtyAntioxidantParinaric Acidmedicine.medical_treatmentOxidative phosphorylationAntioxidantsReference ValuesInternal medicineMedicineHumansPolyacrylamide gel electrophoresisFluorescent DyesIntermediate-density lipoproteinbusiness.industryGeneral MedicineLipoproteins LDLEndocrinologyPhenotypeFatty Acids Unsaturatedlipids (amino acids peptides and proteins)Electrophoresis Polyacrylamide GelFemaleUltracentrifugebusinessQuantitative analysis (chemistry)Oxidation-ReductionLipoproteinThe American journal of medicine
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Nuevas terminaciones para nuevas realidades: performatividad, afiliación y atenuación en la comunidad de habla LGTBI

2021

Este artículo presenta un estudio sobre las terminaciones -i/-is y -e/-es en la comunidad de habla LGTBI. La motivación de esta investigación viene de la representación del género no binario en la lengua española, marcado recientemente por las terminaciones en -e, que además es utilizado para crear un plural inclusivo que evite el masculino genérico. En la misma línea, se han detectado usos, dentro de la comunidad de habla LGTBI, de otro grupo de terminaciones (-i/-is) que parecen anular la distinción de género. Los datos han sido extraídos de una encuesta sociolingüística elaborada por el autor de este trabajo. En la parte sociolingüística se pretende perfilar el tipo de usuario de estas t…

AffiliationLingüística GeneralSpanish languageMitigationGroup (mathematics)AtenuaciónRepresentation (arts)LinguisticsLengua EspañolaNon-binary genderLingüística queerPerformatividadPerformativityQueer linguisticsGénero no binarioPerformativitySociologyAfiliaciónPluralELUA
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Una pedagogia della vita emotiva

2014

Il contributo presenta le linee di una fenomenologa delle emozioni, il cui assunto principale è renderne evidente la portata referenziale. Vengono così giustificate come vie specifiche che consentono la comprensione degli aspetti singolari delle persone che hanno parte ai mondi della nostra vita. È una prospettiva critica rispetto alla cultura che sembra oggi prevalente e che vede invece nelle emozioni quasi esclusivamente il loro aspetto espressivo. Le emozioni come vie di conoscenza hanno poi una loro evoluzione caratteristica, crescendo in consapevolezza e acquistando la dimensione della durata. Viste nelle forme di reazione «favorevole» alla presenza dell’altro sono forme di amore e por…

Alfabetizzazione emotiva Portata referenziale linguaggio originario del corpo Emozioni Affetti Sentimenti culto delle emozioni Empatia Bisogno di riconoscimento DesiderioSettore M-PED/01 - Pedagogia Generale E Sociale
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Breve fenomenologia della vita emotiva nella prospettiva dell'educazione

2018

The paper explores the link between human becoming and biographical narrative, within the empathy-centred existential dialogue. The existential dialogue should not be assimilated to a psychotherapeutic method: it is, rather, a special care relationship within an educational perspective. In a semiological analysis, the existential dialogue is an interaction shaped according to an empathetic code and giving rise to a peculiar relational regulation system based on: 1. demandingness (or control), linked to authority and competence; 2. emotional responsiveness (or empathetic contact), linked to socio-affective interaction; 3. authenticity (or congruence), linked to transparency in speaking. In a…

Alfabetizzazione emotiva linguaggio originario del corpo carattere intenzionale ordo amoris dialogo esistenziale codice empatico bisogno di riconoscimento autorevolezza stile cooperativoSettore M-PED/01 - Pedagogia Generale E Sociale
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