Search results for "Horizontal"

showing 10 items of 251 documents

DISK REFLECTION SIGNATURES IN THE SPECTRUM OF THE BRIGHT Z-SOURCE GX 340+0

2008

We present the preliminary results of a 50 ks long XMM-Newton observation of the bright Z-source GX 340+0. In this Letter we focus on the study of a broad asymmetric emission line in the Fe K alpha energy band, whose shape is clearly resolved and compatible with a relativistically smeared profile arising from reflection on a hot accretion disk extending close to the central accreting neutron star. By combining temporal and spectral analysis, we are able to follow the evolution of the source along its Horizontal Branch. However, despite a significant change in the continuum emission and luminosity, the line profile does not show any strong correlated variation. This broad line is produced by…

PhysicsAstrofisica Alte EnergieAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)Astrofisica Alte Energie;FOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsRadiusAstrophysicsHorizontal branchAstrophysicsGravitationNeutron starSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceIonizationEmissivityK-alphaAstrophysics::Earth and Planetary AstrophysicsEmission spectrumAstrophysics::Galaxy AstrophysicsThe Astrophysical Journal
researchProduct

On the Spectral Evolution of Cygnus X-2 along its Color-Color Diagram

2002

We report on the results of a broad band (0.1-200 keV) spectral study of Cyg X-2 using two BeppoSAX observations taken in 1996 and 1997, respectively, for a total effective on-source time of ~100 ks. The color-color (CD) and hardness-intensity (HID) diagrams show that the source was in the horizontal branch (HB) and normal branch (NB) during the 1996 and 1997 observation, respectively. Five spectra were selected around different positions of the source in the CD/HID, two in the HB and three in the NB. These spectra are fit to a model consisting of a disk blackbody, a Comptonization component, and two Gaussian emission lines at ~1 keV and ~6.6 keV, respectively. The addition of a hard power-…

PhysicsAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)FOS: Physical sciencesAstronomy and AstrophysicsColor–color diagramAstrophysicsRadiusHorizontal branchaccretion accretion disks / stars: individual: Cyg X–2 / stars: neutron / X-rays: stars / X-rays: binaries / X-rays: generalAstrophysicsSpectral lineLuminosityNOaccretionSpace and Planetary ScienceOptical depth (astrophysics)accretion disks / stars: individual: Cyg X–2 / stars: neutron / X-rays: stars / X-rays: binaries / X-rays: generalElectron temperatureEmission spectrum
researchProduct

Presymplectic manifolds and conservation laws

2008

In this paper we make use of a new structure called seeded fibre bundle. This allows us to combine the symplectic formalism and general relativity. A theorem of existence is obtained and some examples and properties are studied.

PhysicsFormalism (philosophy of mathematics)Pure mathematicsConservation lawMathematics::Algebraic GeometryGeneral relativityFiber bundleHorizontal distributionMathematics::Symplectic GeometryMathematical physicsFibre typeSymplectic manifoldSymplectic geometry
researchProduct

Patterns of variability in Be/X-ray pulsars during giant outbursts

2012

The discovery of source states in the X-ray emission of black-hole binaries and neutron-star low-mass X-ray binaries constituted a major step forward in the understanding of the physics of accretion onto compact objects. While there are numerous studies on the correlated timing and spectral variability of these systems, very little work has been done on high-mass X-ray binaries, the third major type of X-ray binaries. The main goal of this work is to investigate whether Be accreting X-ray pulsars display source states and characterise those states through their spectral and timing properties. We have made a systematic study of the power spectra, energy spectra and X-ray hardness-intensity d…

PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)Astrophysics::High Energy Astrophysical PhenomenaFluxFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsHorizontal branchCritical valueSpectral lineLuminosityPulsarSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaNoise (radio)
researchProduct

Study of Two BeppoSAX Observations of GX 340+0

2006

We present the results of two BeppoSAX broad band (0.1–200 keV) observations of the Z-source GX 340+0 comparing our results to those of a previous observation of the source. From the color–color diagram we selected three zones and extracted the source energy spectrum from each zone. We find that the model, composed by a blackbody plus a Comptonized component, absorbed by an equivalent hydrogen column of ~6 × 10 22 cm −2 , well fits the spectra in the energy range below 30 keV. At higher energies a power law component with photon index of 2.5 is observed. The associated flux decreases going from the horizontal branch to the flaring branch of the Z-track.

PhysicsRange (particle radiation)PhotonHydrogenAstrophysics::High Energy Astrophysical PhenomenaFluxAstronomychemistry.chemical_elementAstronomy and Astrophysicsstars : individual (GX 340+0)AstrophysicsHorizontal branchindividual (GX 340+0); X-rays : binaries; X-rays : general [stars]Power lawSpectral linechemistrySpace and Planetary ScienceBlack-body radiationX-rays : binarieX-rays : generalChinese Journal of Astronomy and Astrophysics
researchProduct

Self-Enrichment in Globular Clusters: Is There a Role for the Super-Asymptotic Giant Branch Stars?

2008

In four globular clusters (GCs) a non negligible fraction of stars can be interpreted only as a very helium rich population. The evidence comes from the presence of a "blue" main sequence in $\omega$ Cen and NGC 2808, and from the the very peculiar horizontal branch morphology in NGC 6441 and NGC 6388. Although a general consensus is emerging on the fact that self--enrichment is a common feature among GCs, the helium content required for these stars is Y$\simgt$0.35, and it is difficult to understand how it can be produced without any --or, for $\omega$ Cen, without a considerable--associated metal enhancement. We examine the possible role of super--AGB stars, and show that they may provide…

Physicseducation.field_of_studyAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)PopulationFOS: Physical sciencesWhite dwarfAstronomy and AstrophysicsAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsHorizontal branchDredge-upAstrophysicsStarsNeutron starSpace and Planetary ScienceGlobular clusterAsymptotic giant branchAstrophysics::Solar and Stellar AstrophysicseducationAstrophysics::Galaxy Astrophysics
researchProduct

Real-time Sub-pixel Cross Bar Position Metrology

2002

Many measurement application fields need to calculate cross bar intersection locations of horizontal and vertical bars. The system we developed and that we present in this paper is an embedded system that measures cross bar positions with sub-pixel accuracy on 1024×1024 pixel images delivered by a camera at a 50 MHz data rate in real time. This is done using an algorithm that looks for intersection areas and then locally calculates two lines representing horizontal and vertical bars. The two line intersection is considered to be the bar intersection. To achieve real time, we developed a hybrid architecture in which low level processes are implemented into FPGAs and others into DSPs. As a re…

PixelHorizontal and verticalComputer sciencebusiness.industryBar (music)MetrologyIntersectionLine–line intersectionPosition (vector)Embedded systemSignal ProcessingComputer visionComputer Vision and Pattern RecognitionArtificial intelligenceElectrical and Electronic EngineeringbusinessField-programmable gate arrayReal-Time Imaging
researchProduct

A Tomographical Characterization of L-convex Polyominoes

2005

Our main purpose is to characterize the class of L-convex polyominoes introduced in [3] by means of their horizontal and vertical projections. The achieved results allow an answer to one of the most relevant questions in tomography i.e. the uniqueness of discrete sets, with respect to their horizontal and vertical projections. In this paper, by giving a characterization of L-convex polyominoes, we investigate the connection between uniqueness property and unimodality of vectors of horizontal and vertical projections. In the last section we consider the continuum environment; we extend the definition of L-convex set, and we obtain some results analogous to those for the discrete case.

Pure mathematicsInteger VectorHorizontal and verticalPolyominoDiscrete TomographyConvex setDiscrete geometryUnimodalityConnection (mathematics)Vertical ProjectionContinuum CounterpartMonotone PathUniquenessDiscrete tomographyMathematics
researchProduct

Simultaneous occurrence of covert infections with small RNA viruses in the lepidopteran Spodoptera exigua

2014

Viral covert infections in invertebrates have been traditionally attributed to sublethal infections that were not able to establish an acute infection. Recent studies are revealing that, although true for some viruses, other viruses may follow the strategy of establishing covert or persistent infections without producing the death of the host. Recently, and due to the revolution in the sequencing technologies, a large number of viruses causing covert infections in all type of hosts have been identified.The beet armyworm, Spodoptera exigua (Lepidoptera: Noctuidae) is a worldwide pest that causes significant losses to agricultural and ornamental plant industries. In a previous project we used…

RNA virusvirusesGenome ViralSpodopteraPersistent infectionVirusVirus morphologySpodoptera exiguaExiguaCovert infectionsAnimalsRNA VirusesEcology Evolution Behavior and SystematicsPhylogenybiologyHost (biology)IflavirusfungiPicornaviralesRNA virusbiology.organism_classificationVirologyIflaviridaeHost-Pathogen InteractionsPicornaviralesHorizontal transmission
researchProduct

Displacement Evolution of a Large Landslide in a Highly Fissured Clay

2019

The paper presents an analysis and modelling of the reactivation mechanism of a large landslide caused by rainfall, located in Cerda (Sicily, Italy). The study is based on data collected by means of a field investigation, carried out in order to assess the geotechnical properties of the involved material, and a three-year monitoring programme implemented to measure rain and pore water pressures as well as deep and superficial displacements. Three distinct landslides, evolving at variable rates in different directions, were recognized within the overall landslide area. The data clearly show the mechanical role of pore water pressures in the stability of the slope and point out the dependence…

RainfallPore water pressureLandslideSettore ICAR/07 - GeotecnicaHorizontal displacementTime evolutionFissured clayGeotechnical engineeringLandslideSlip (materials science)ModellingGeology
researchProduct