Search results for "SCS"

showing 10 items of 157 documents

The jets and disc of SS 433 at super-Eddington luminosities

2009

We examine the jets and the disc of SS 433 at super-Eddington luminosities with 600 times Eddington critical accretion rate by time-dependent two-dimensional radiation hydrodynamical calculations, assuming alpha-model for the viscosity. One-dimensional supercritical accretion disc models with mass loss or advection are used as the initial configurations of the disc. As a result, from the initial advective disc models with alpha =0.001 and 0.1, we obtain the total luminosities 2.5x10^{40} and 2.0x10^{40} erg/s. The total mass-outflow rates are 4x10^{-5} and 10^{-4} solar-mass/yr and the rates of the relativistic axial outflows in a small half opening angle of 1 degree are about 10^{-6} solar…

High Energy Astrophysical Phenomena (astro-ph.HE)Physicsaccretion accretion discs black hole physics hydrodynamics radiation mechanisms: thermal X-rays: individual: SS 433Jet (fluid)Plane (geometry)AdvectionAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsRadiationLuminosityViscositySettore FIS/05 - Astronomia E AstrofisicaAmplitudeSpace and Planetary ScienceAstrophysics::Solar and Stellar AstrophysicsOutflowAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy AstrophysicsMonthly Notices of the Royal Astronomical Society
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Testing Rate Dependent corrections on timing mode EPIC-pn spectra of the accreting Neutron Star GX 13+1

2014

When the EPIC-pn instrument on board XMM-Newton is operated in Timing mode, high count rates (>100 cts/s) of bright sources may affect the calibration of the energy scale, resulting in a modification of the real spectral shape. The corrections related to this effect are then strongly important in the study of the spectral properties. Tests of these calibrations are more suitable in sources which spectra are characterised by a large number of discrete features. Therefore, in this work, we carried out a spectral analysis of the accreting Neutron Star GX 13+1, which is a dipping source with several narrow absorption lines and a broad emission line in its spectrum. We tested two different co…

High Energy Astrophysical Phenomena (astro-ph.HE)Physicsaccretion accretion discs line: identification stars: neutron X-rays: binaries X-rays: galaxies X-rays: individual: (GX 13+1)Spectral shape analysisAccretion (meteorology)Absorption spectroscopyAstrophysics::High Energy Astrophysical PhenomenaContinuum (design consultancy)FOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsAstrophysics - Astrophysics of GalaxiesSpectral lineNeutron starAmplitudeidentification stars: neutron X-rays: binaries X-rays: galaxies X-rays: individual: (GX 13+1) [accretion accretion discs line]Settore FIS/05 - Astronomia E AstrofisicaSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Emission spectrumAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)
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The pulse profile and spin evolution of the accreting pulsar in Terzan 5, IGR J17480-2446, during its 2010 outburst

2012

(abridged) We analyse the spectral and pulse properties of the 11 Hz transient accreting pulsar, IGR J17480-2446, in the globular cluster Terzan 5, considering all the available RXTE, Swift and INTEGRAL observations performed between October and November, 2010. By measuring the pulse phase evolution we conclude that the NS spun up at an average rate of =1.48(2)E-12 Hz/s, compatible with the accretion of the Keplerian angular momentum of matter at the inner disc boundary. Similar to other accreting pulsars, the stability of the pulse phases determined by using the second harmonic component is higher than that of the phases based on the fundamental frequency. Under the assumption that the sec…

High Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/05 - Astronomia E AstrofisicaAstrophysics::High Energy Astrophysical Phenomenaneutron pulsars: individual: IGR J17480-2446 X-rays: binaries [accretion accretion discs stars]FOS: Physical sciencesAstrophysics::Solar and Stellar Astrophysicsaccretion accretion discs stars: neutron pulsars: individual: IGR J17480-2446 X-rays: binariesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaAstrophysics::Galaxy Astrophysics
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Unveiling the disc structure in ultraluminous X-ray source NGC 55 ULX-1

2022

Ultraluminous X-ray sources (ULXs) are the most extreme among X-ray binaries in which the compact object, a neutron star or a black hole, accretes matter from the companion star, and exceeds a luminosity of 1039 ergs−1 in the X-ray energy band alone. Despite two decades of studies, it is still not clear whether ULX spectral transitions are due to stochastic variability in the wind or variations in the accretion rate or in the source geometry. The compact object is also unknown for most ULXs. In order to place constraints on to such scenarios and on the structure of the accretion disc, we studied the temporal evolution of the spectral components of the variable source NGC 55 ULX-1. Using rec…

High Energy Astrophysical Phenomena (astro-ph.HE)X-rays: binariesAccretionSettore FIS/05 - Astronomia E AstrofisicaSpace and Planetary Scienceaccretion discFOS: Physical sciencesAstronomy and AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaX-rays: binarieX-rays: individual: NGC 55 ULX-1Accretion discs
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MAXI J1957+032: a new accreting millisecond X-ray pulsar in an ultra-compact binary

2022

The detection of coherent X-ray pulsations at ~314 Hz (3.2 ms) classifies MAXI J1957+032 as a fast-rotating, accreting neutron star. We present the temporal and spectral analysis performed using NICER observations collected during the latest outburst of the source. Doppler modulation of the X-ray pulsation revealed the ultra-compact nature of the binary system characterised by an orbital period of ~1 hour and a projected semi-major axis of 14 lt-ms. The neutron star binary mass function suggests a minimum donor mass of 1.7e-2 Msun, assuming a neutron star mass of 1.4 Msun and a binary inclination angle lower than 60 degrees. This assumption is supported by the lack of eclipses or dips in th…

High Energy Astrophysical Phenomena (astro-ph.HE)general–stars:neutron [Binaries]FOS: Physical sciencesAstronomy and Astrophysicsaccretion discsbinaries:generalX-rays:binariesSettore FIS/05 - Astronomia E AstrofisicaaccretionSpace and Planetary Sciencebinaries [X-rays]stars:neutronAstrophysics - High Energy Astrophysical PhenomenaAstrophysics - Instrumentation and Methods for AstrophysicsInstrumentation and Methods for Astrophysics (astro-ph.IM)accretion disks [Accretion]
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Mutant p53 gain of function can be at the root of dedifferentiation of human osteosarcoma MG63 cells into 3AB-OS cancer stem cells

2014

Osteosarcoma is a highly metastatic tumor affecting adolescents, for which there is no second-line chemotherapy. As suggested for most tumors, its capability to overgrow is probably driven by cancer stem cells (CSCs), and finding new targets to kill CSCs may be critical for improving patient survival. TP53 is the most frequently mutated tumor suppressor gene in cancers and mutant p53 protein (mutp53) can acquire gain of function (GOF) strongly contributing to malignancy. Studies thus far have not shown p53-GOF in osteosarcoma. Here, we investigated TP53 gene status/role in 3AB-OS cells-a highly aggressive CSC line previously selected from human osteosarcoma MG63 cells-to evaluate its involv…

HistologyTumor suppressor genePhysiologyEndocrinology Diabetes and MetabolismApoptosisIn situ hybridizationBiologyTNF-Related Apoptosis-Inducing LigandCell MovementCancer stem cellCell Line TumorSettore BIO/10 - BiochimicaBiomarkers TumormedicineHumansNeoplasm Invasiveness3AB-OS cells CSCs Cancer cell dedifferentiation Cancer stem cells FISH Fluorescent in situ hybridization GOF Gain of function Human osteosarcoma MMPs Matrix metalloproteinases Mutant p53 Mutant p53 gain of function Mutp53 OS OsteosarcomaClonogenic assayTumor Stem Cell AssayCell ProliferationMembrane Potential MitochondrialOsteosarcomaCancerReceptors Death DomainCell DedifferentiationCell cyclemedicine.diseaseMolecular biologyAmino Acid SubstitutionProto-Oncogene Proteins c-bcl-2Gene Knockdown TechniquesMutationNeoplastic Stem CellsCancer researchOsteosarcomaEctopic expressionTumor Suppressor Protein p53Bone
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Síntesis de los estudios sobre moluscos continentales neógenos del sector septentrional de la Depresión de Teruel: período 1775-1998

2006

Se recopila y analiza la información que se considera más relevante y se encuentra contenida en los estudios realizados sobre el registro fósil de los moluscos neógenos del sector septentrional de la Depresión de Teruel en el período comprendido entre los años 1775 y 1998. Se contabilizan, por una parte, el número total de taxones diferentes mencionados en cada trabajo y, por otra, sólo el número de citas efectuadas a nivel de especie en cada uno de ellos. Estas últimas se organizan en tres categorías que reciben el nombre de citas nuevas, especies nuevas y citas repetidas. Se propone, a partir de la información contenida en cada trabajo, el número de taxones contemplados, y la tipología de…

Historia de la Paleontología; Moluscos continentales; Neógeno; Depresión de Teruel; EspañaMoluscos continentaleshistoria de la paleontologíaespañaQE1-996.5Historia de la PaleontologíaEspañaTeruel BasinGeologyDepresión de TeruelUNESCO::CIENCIAS DE LA TIERRA Y DEL ESPACIO::Geología:CIENCIAS DE LA TIERRA Y DEL ESPACIO::Geología [UNESCO]Neógenodepresión de teruelSpainHistory of Palaeontologymoluscos continentalesContinental molluscsNeogeneneógeno
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Inbreeding does not alter the response to an experimental heat wave in a freshwater snail

2019

Global climate change affects natural populations of many species by increasing the average temperature and the frequency of extreme weather events (e.g. summer heat waves). The ability of organisms to cope with these environmental changes can, however, depend on their genetic properties. For instance, genetic load owing to inbreeding could alter organisms’ responses to climate change-mediated environmental changes but such effects are often overlooked. We investigated the effects of an experimental heat wave (25°C versus 15°C) on life history (reproduction, size) and constitutive immune defence traits (phenoloxidase-like and antibacterial activity of haemolymph) in relation to inbreeding b…

Hot TemperatureHeredityPhysiologyOvipositionSnailsMarine and Aquatic SciencesMathematical and Statistical TechniquesReproductive PhysiologyMedicine and Health SciencesBody SizeInbreedingImmune ResponseLymnaeaAntimicrobialsReproductionStatisticsQREukaryotaDrugsimmuunivastePhysical SciencesMedicinelämpötilaClutchesympäristönmuutoksetResearch ArticleClimate ChangeScienceImmunologyResearch and Analysis MethodsMicrobiologyMicrobial ControlGeneticsAnimalsLymnaea stagnalisStatistical MethodsPondsPharmacologyEvolutionary BiologyAnalysis of VariancePopulation BiologyfungivesikotilotImmunityOrganismsBiology and Life SciencesMolluscsBodies of WaterilmastonmuutoksetlisääntyminenInvertebratespiippolimakotiloGastropodsEarth SciencesGenetic PolymorphismsukusiitosAntibacterialsPopulation GeneticsMathematics
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SCS Curve Number and Green-Ampt Infiltration Models

2019

Soil Conservation Service curve number (SCS-CN) and Green-Ampt (GA) infiltration models are probably the most applied equations in practical hydrology to compute the amount of direct runoff from rainfall. Both models are very simple, require few parameters, and present drawbacks and advantages. The empirical CN model concentrates the infiltration effect in the curve number and in the so-called soil hydrological groups, which have been widely characterized for different soil types, land cover, and antecedent soil moisture conditions (ASMCs), although the latter was considered ambiguous, whereas soil hydrological characteristics, including ASMC, are taken into account for the simplified physi…

Hydrology010504 meteorology & atmospheric sciencesGreen-Ampt model0208 environmental biotechnologySCS-CN model02 engineering and technologyRunoff curve numberinfiltration01 natural sciences020801 environmental engineeringAMPTInfiltration (hydrology)medicineSettore AGR/08 - Idraulica Agraria E Sistemazioni Idraulico-ForestaliEnvironmental ChemistryEnvironmental scienceSurface runoff0105 earth and related environmental sciencesGeneral Environmental ScienceWater Science and TechnologyCivil and Structural Engineeringmedicine.drugJournal of Hydrologic Engineering
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The Challenge of Using CB-HSCs As Source for Gene Therapy: Lentiviral Vector Transduction, Phenotypic Characterization and Global Gene Expression Pro…

2015

Abstract Introduction: Genetic modification of autologous hematopoietic stem and progenitor cells (HSPC) is a promising clinical intervention to cure inherited monogenic diseases. Successful gene therapy trials have already been conducted using CD34+ cells from bone marrow and from mobilized peripheral blood. In this regard, cord blood (CB) represents an attractive source of HSCs due to its high concentration of high proliferative HSPC and increased susceptibility to be transduced by lentiviral vectors. Unfortunately, the major disadvantage is the limited number of HSC in the CB collection. Consequently, ex-vivo expansion of CB-HSC is desirable to extend clinical applications. Purposes: To …

ImmunologyCD34Cell BiologyHematologyBiologyCD38BiochemistryMolecular biologyViral vectorGene expression profilingHaematopoiesisSettore BIO/18 - GeneticaCB-HSCs Gene Therapy Gene Expression Profile of Ex-Vivo Expanded CB CD34+ Cells.Cell cultureImmunologyProgenitor cellInterleukin 3
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