Search results for "CCR"

showing 10 items of 574 documents

A TEST of the NATURE of the FE K LINE in the NEUTRON STAR LOW-MASS X-RAY BINARY SERPENS X-1

2015

Broad Fe K emission lines have been widely observed in the X-ray spectra of black hole systems, and in neutron star systems as well. The intrinsically narrow Fe K fluorescent line is generally believed to be part of the reflection spectrum originating in an illuminated accretion disk, and broadened by strong relativistic effects. However, the nature of the lines in neutron star LMXBs has been under debate. We therefore obtained the longest, high-resolution X-ray spectrum of a neutron star LMXB to date with a 300 ks Chandra HETGS observation of Serpens X-1. The observation was taken under the "continuous clocking" mode and thus free of photon pile-up effects. We carry out a systematic analys…

SerpensAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesAstrophysicsaccretion accretion disk01 natural sciencesSpectral linestars: neutronSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesEmission spectrum010303 astronomy & astrophysicsLine (formation)High Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsAstronomy and Astrophysicsprofiles; stars: neutron; X-rays: binaries; Astronomy and Astrophysics; Space and Planetary Science [accretion accretion disks; line]Astronomy and AstrophysicK-lineX-rays: binarieBlack holeNeutron starline: profileSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena
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From Cash to Accrual Accounting: The seminal case of the Sicilian Regional Public Bodies

2019

The Italian public sector has been traditionally characterised by a cash-based and compliance-oriented governmental accounting, principally aimed at supporting the budgetary control by the legislative body. Over the last few decades, however, a new movement has been spreading around the world, casting doubt on the potentialities and advantages of the traditional accounting system in favour of an accrual basis one. This paper traces the progressive introduction of a complete accrual accounting by the Sicilian Regional public bodies – within the context of international and national public management changes – pursuing the ultimate goal to improve efficiency, accountability and transparency. …

Settore SECS-P/07 - Economia AziendaleNPM accrual accounting chart of accounts Sicilian Regional public bodies public value
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Global Soil Biodiversity Atlas

2016

SPE EA Pôle BIOME The Atlas is divided in 8 chapters covering all the aspects of soil biodiversity: - Chapter I: The soil habitat - Chapter II: Diversity of soil organisms - Chapter III: Geographical and temporal distribution - Chapter IV: Ecosystem functions and services - Chapter V: Threats - Chapter VI: Interventions - Chapter VII: Policy, education and outreach - Chapter VIII: Conclusions Soil biodiversity experts from all over the world are involved in the project aiming at the creation of a reference publication not only for soil biodiversity researchers but also policy makers and general public.; International audience; The Global Soil Biodiversity Initiative (GSBI) and the Joint Res…

[SDV] Life Sciences [q-bio][SDE] Environmental SciencesCentre Commun de Recherche[SDV]Life Sciences [q-bio]JRC[SDE]Environmental SciencesGlobal Soil Biodiversity Initiative[SDV.BV]Life Sciences [q-bio]/Vegetal Biology[SDV.BV] Life Sciences [q-bio]/Vegetal BiologyEuropean CommissionCCRGSBI
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La interpretación judicial en España en un momento de cambio.

2015

The publication in the European Union of Directive 2010/64/EU of the European Parliament and of the Council of 20 October 2010 on the right to interpretation and translation in criminal proceedings has been a turning point in a great number of aspects related to court and police interpretation. The main objective of the Directive is to ensure quality legal interpretation throughout the process, as part of the right to defense and to a fair trial. Spain, as a Member State of the EU, has the obligation to transpose this European Directive into its domestic law. Therefore, this is a historic moment in which two main factors converge: the need to change the legislation to bring it in line with …

Linguistics and Languageinterpretación judiciallegal interpretingParliamentmedia_common.quotation_subjectLegislationPublic administrationLanguage and LinguisticsaccreditationEducationprofesionalizaciónformaciónPolitical scienceprofessionalizationMember statemedia_common.cataloged_instanceDirective on Privacy and Electronic Communicationslegal interpreting; professionalization; training; accreditation; registerObligationEuropean unionmedia_commonUNESCO::CIENCIAS DE LAS ARTES Y LAS LETRASregistertrainingTraducción e Interpretacióninterpretación judicial; profesionalización; formación; acreditación; registroMunicipal lawDirectiveregistroacreditaciónLaw:CIENCIAS DE LAS ARTES Y LAS LETRAS [UNESCO]
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Systemic Immune Responses in Alzheimer's Disease: In Vitro Mononuclear Cell Activation and Cytokine Production

2010

To investigate the systemic signs of immune-inflammatory responses in Alzheimer's disease (AD), in the present study we have analyzed blood lymphocyte subsets and the expression of activation markers on peripheral blood mononuclear cells (PBMCs) from AD patients and age-matched healthy controls (HC) activated in vitro by recombinant amyloid-beta peptide (rAbeta42). Our study of AD lymphocyte subpopulations confirms the already described decrease of the absolute number and percentage of B cells when compared to HC lymphocytes, whereas the other subsets are not significantly different in patients and controls. We report the increased expression of the activation marker CD69 and of the chemoki…

MaleEotaxinCCR2ChemokineTime Factorsmedicine.medical_treatmentPeripheral blood mononuclear cellChemokine receptorImmune systemAlzheimer’s disease chemokine cytokine PBMC rAβ42Alzheimer DiseasemedicineHumansLymphocytesIL-2 receptorCells CulturedAgedSettore MED/04 - Patologia GeneraleAged 80 and overAnalysis of VarianceAmyloid beta-Peptidesbiologybusiness.industryGeneral NeuroscienceGeneral MedicineMiddle AgedFlow CytometryPeptide FragmentsPsychiatry and Mental healthClinical PsychologyCytokineGene Expression RegulationCase-Control StudiesImmunologyLeukocytes Mononuclearbiology.proteinCytokinesFemaleGeriatrics and GerontologybusinessJournal of Alzheimer's Disease
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Harmonic Coupling of the Red Noise in X‐Ray Pulsars

1997

The power spectra of X-ray pulsars often show the presence of a red-noise component. This noise is produced by aperiodic variability believed to be associated with instabilities that seem to occur in accretion flows onto compact objects. In this paper we discuss how, independently of the details of the physical processes that generate these instabilities, a careful analysis of the power spectra can furnish some constraints on the distance from the stellar surface at which the sudden energy release associated with the instabilities occurs. In particular, any aperiodic variability coming from the accretion flow funneled toward the magnetic poles should be modulated at the pulsar spin period (…

PhysicsPulsarSpace and Planetary ScienceColors of noiseAperiodic graphHarmonicsX-rayAstronomy and AstrophysicsAstrophysicsLight curveAccretion (astrophysics)Spectral lineThe Astrophysical Journal
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Radiative accretion shocks along nonuniform stellar magnetic fields in classical T Tauri stars

2013

(abridged) AIMS. We investigate the dynamics and stability of post-shock plasma streaming along nonuniform stellar magnetic fields at the impact region of accretion columns. We study how the magnetic field configuration and strength determine the structure, geometry, and location of the shock-heated plasma. METHODS. We model the impact of an accretion stream onto the chromosphere of a CTTS by 2D axisymmetric magnetohydrodynamic simulations. Our model takes into account the gravity, the radiative cooling, and the magnetic-field-oriented thermal conduction. RESULTS. The structure, stability, and location of the shocked plasma strongly depend on the configuration and strength of the magnetic f…

Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesField strengthX-rays: starsAstrophysicsstars: pre-main sequence01 natural sciencesmagnetohydrodynamics (MHD)pre-main sequence X-rays: stars [accretion accretion disks instabilities magnetohydrodynamics (MHD) shock waves stars]010305 fluids & plasmasSettore FIS/05 - Astronomia E Astrofisicaaccretion0103 physical sciencesRadiative transferAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysicsaccretion disksAstronomy and AstrophysicsPlasmashock wavesAccretion (astrophysics)Magnetic fieldT Tauri starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceinstabilitiesPhysics::Space PhysicsOblique shockAstrophysics::Earth and Planetary Astrophysicsaccretion accretion disks instabilities magnetohydrodynamics (MHD) shock waves stars: pre-main sequence X-rays: stars[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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The Origin of T Tauri X-ray Emission: New Insights from the Chandra Orion Ultradeep Project

2005

We use the data of the Chandra Orion Ultradeep Project (COUP) to study the nearly 600 X-ray sources that can be reliably identified with optically well characterized T Tauri stars (TTS) in the Orion Nebula Cluster. We detect X-ray emission from more than 97% of the optically visible late-type (spectral types F to M) cluster stars. This proofs that there is no ``X-ray quiet'' population of late-type stars with suppressed magnetic activity. All TTS with known rotation periods lie in the saturated or super-saturated regime of the relation between activity and Rossby numbers seen for main-sequence (MS) stars, but the TTS show a much larger scatter in X-ray activity than seen for the MS stars. S…

Physicseducation.field_of_studyAstrophysics::High Energy Astrophysical PhenomenaPopulationAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsStellar classificationAstrophysicsSpectral lineAccretion (astrophysics)LuminosityStarsT Tauri starSpace and Planetary ScienceOrion NebulaAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicseducationAstrophysics::Galaxy Astrophysics
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Structural overprint of a late Paleozoic accretionary system in north-central Chile (34°-35°S) during post-accretional deformation

2009

En la Cordillera de la Costa de Chile, de 36° a 35°S, se encuentra expuesta la arquitectura coherentemente preservada de un prisma de acrecion del Paleozoico tardio, en cercana vecindad a un area entre los 34° y 35°S, donde el mismo esta fuertemente modificado por procesos postacrecionales. Estudiando las desviaciones de la arquitectura original, en esta region pueden ser perfectamente distinguidas estructuras sin- y post acrecionales. Al sur de los 35° se observa un contacto transicional entre dos unidades mayores, el cual refleja un cambio continuo en el modo de acrecion de la cuna acrecional antes de -305 Ma: las metagrauvacas estructuralmente suprayacentes de las series orientales muest…

Post-accretional deformationSubduction erosiónAccretionary prismNorth centralStratigraphyBasal accretionPaleontologyMineralogyGeologyFrontal accretionStrike-slipGeochemistry and PetrologyReverse faultLate PaleozoicHumanitiesGeologyAndean geology
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A Decade in the Life of EXO 2030+375: A Multiwavelength Study of an Accreting X‐Ray Pulsar

2002

Using BATSE and RXTE observations from 1991 April to 2001 August we have detected 71 outbursts from 82 periastron passages of EXO 2030+375, a 42-second transient X-ray pulsar with a Be star companion, including several outbursts from 1993 August to 1996 April when the source was previously believed to be quiescent. Combining BATSE, RXTE, and EXOSAT data we have derived an improved orbital solution. Applying this solution results in a smooth profile for the spin-up rate during the giant outburst and results in evidence for a correlation between the spin-up rate and observed flux in the brighter BATSE outbursts. Infrared and Halpha measurements show a decline in the density of the circumstell…

PhysicsBe starOscillationAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Phase (waves)FOS: Physical sciencesFluxAstronomy and AstrophysicsMulti wavelengthAstrophysicsAstrophysicsAccretion discPulsarSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Galaxy AstrophysicsX-ray pulsarThe Astrophysical Journal
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