Search results for "Star"

showing 10 items of 4285 documents

On the timing properties of SAX J1808.4-3658 during its 2015 outburst

2017

We present a timing analysis of the 2015 outburst of the accreting millisecond X-ray pulsar SAX J1808.4-3658, using non-simultaneous XMM-Newton and NuStar observations. We estimate the pulsar spin frequency and update the system orbital solution. Combining the average spin frequency from the previous observed, we confirm the long-term spin down at an average rate $\dot{\nu}_{\text{SD}}=1.5(2)\times 10^{-15}$ Hz s$^{-1}$. We also discuss possible corrections to the spin down rate accounting for mass accretion onto the compact object when the system is X-ray active. Finally, combining the updated ephemerides with those of the previous outbursts, we find a long-term orbital evolution compatibl…

Angular momentumAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesLagrangian pointAstrophysicsCompact star01 natural sciencespulsars: individual: SAX J1808.4-3658Gravitationstars: neutronX-rays: binariesSettore FIS/05 - Astronomia E AstrofisicaPulsar0103 physical sciences010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsOrbital periodaccretion accretion discs; stars: neutron; pulsars: individual: SAX J1808.4-3658; X-rays: binaries13. Climate actionSpace and Planetary ScienceQuadrupole:accretion accretion discAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Relativistic simulations of rotational core collapse : I. Methods, initial models, and code tests

2002

We describe an axisymmetric general relativistic code for rotational core collapse. The code evolves the coupled system of metric and fluid equations using the ADM 3+1 formalism and a conformally flat metric approximation of the Einstein equations. The relativistic hydrodynamics equations are formulated as a first-order flux-conservative hyperbolic system and are integrated using high-resolution shock-capturing schemes based on Riemann solvers. We assess the quality of the conformally flat metric approximation for relativistic core collapse and present a comprehensive set of tests which the code successfully passed. The tests include relativistic shock tubes, the preservation of the rotatio…

Angular momentumAstrophysics::High Energy Astrophysical PhenomenaRotational symmetryFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)AstrophysicsNumerical methodAstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICAGeneral Relativity and Quantum CosmologyGravitational wavesGravitationRelativitysymbols.namesakeWaveformPhysicsAstrophysics (astro-ph)Astronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]Hyperbolic systemsNeutron starRiemann hypothesisClassical mechanicsSpace and Planetary ScienceGravitational waves ; Hydrodynamics ; Numerical method ; RelativitysymbolsHydrodynamicsFluid equationUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Mass Accretion Processes in Young Stellar Objects: Role of Intense Flaring Activity

2014

According to the magnetospheric accretion scenario, young low-mass stars are surrounded by circumstellar disks which they interact with through accretion of mass. The accretion builds up the star to its final mass and is also believed to power the mass outflows, which may in turn have a significant role in removing the excess angular momentum from the star-disk system. Although the process of mass accretion is a critical aspect of star formation, some of its mechanisms are still to be fully understood. On the other hand, strong flaring activity is a common feature of young stellar objects (YSOs). In the Sun, such events give rise to perturbations of the interplanetary medium. Similar but mo…

Angular momentumMHDStars: flareAstrophysics::High Energy Astrophysical PhenomenaYoung stellar objectFOS: Physical sciencesInterplanetary mediumAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAcoustics and UltrasonicAccretion accretion diskIntermediate polarAstrophysics::Solar and Stellar AstrophysicsX-rays: starSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsNuclear and High Energy PhysicGeneral Environmental SciencePhysicsRadiationStar formationAstronomyAccretion (astrophysics)StarsAstrophysics - Solar and Stellar Astrophysicslcsh:TA1-2040Space and Planetary ScienceStars: circumstellar matterGeneral Earth and Planetary SciencesCircumstellar dustAstrophysics::Earth and Planetary Astrophysicslcsh:Engineering (General). Civil engineering (General)Stars: pre-main-sequenceActa Polytechnica CTU Proceedings
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A stellar flare-coronal mass ejection event revealed by X-ray plasma motions

2019

Coronal mass ejections (CMEs), often associated with flares, are the most powerful magnetic phenomena occurring on the Sun. Stars show magnetic activity levels up to 10^4 times higher, and CME effects on stellar physics and circumstellar environments are predicted to be significant. However, stellar CMEs remain observationally unexplored. Using time-resolved high-resolution X-ray spectroscopy of a stellar flare on the active star HR 9024 observed with Chandra/HETGS, we distinctly detected Doppler shifts in S XVI, Si XIV, and Mg XII lines that indicate upward and downward motions of hot plasmas (~10-25 MK) within the flaring loop, with velocity v~100-400 km/s, in agreement with a model of fl…

Angular momentumX-ray Astronomy010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaStars: flareFOS: Physical sciencesAstrophysicsKinetic energy01 natural scienceslaw.inventionSpitzer Space Telescopelaw0103 physical sciencesCoronal mass ejectionAstrophysics::Solar and Stellar AstrophysicsStars: coronae010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciencesLine (formation)PhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astronomy and AstrophysicsStarsAstrophysics - Solar and Stellar AstrophysicsStellar physicsPhysics::Space PhysicsStars: CMEAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFlare
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Evolutionary paths of binaries with a neutron star - I. The case of SAX J1808.4 - 3658

2018

The evolutionary status of the low mass X-ray binary SAX J1808.4-3658 is simulated by following the binary evolution of its possible progenitor system through mass transfer, starting at a period of $\sim$6.6 hr. The evolution includes angular momentum losses via magnetic braking and gravitational radiation. It also takes into account the effects of illumination of the donor by both the X-ray emission and the spin down luminosity of the pulsar. The system goes through stages of mass transfer and stages during which it is detached, where only the rotationally powered pulsar irradiates the donor. We show that the pulsar irradiation is a necessary ingredient to reach SAX J1808.4-3658 orbital pe…

Angular momentumastro-ph.SRAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics01 natural sciencesLuminosityPulsars: individual: SAX J1808.4Settore FIS/05 - Astronomia E AstrofisicaPulsarBinaries: closeMass transfer0103 physical sciencesBinaries: generalStars: low-maAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)3658 -X-rays: binarieHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicsastro-ph.HE010308 nuclear & particles physicsGravitational waveAstronomy and AstrophysicsAstronomy and AstrophysicOrbital periodNeutron starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceAstrophysics - High Energy Astrophysical PhenomenaLow Mass
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A preliminary study in Wistar rats with enniatin : A contaminated feed

2014

A 28-day repeated dose preliminary assay, using enniatin A naturally contaminated feed through microbial fermentation by a Fusarium tricinctum strain, was carried out employing two months-old female Wistar rats as in vivo experimental model. In order to simulate a physiological test of a toxic compound naturally produced by fungi, five treated animals were fed during twenty-eight days with fermented feed. As control group, five rats were fed with standard feed. At the 28th day, blood samples were collected for biochemical analysis and the gastrointestinal tract, liver and kidneys were removed from each rat for enniatin A detection and quantitation. Digesta were collected from stomach, duode…

Animal feedHealth Toxicology and MutagenesisIleumFood ContaminationBiologyToxicologyCromatografia de líquidsIntestinal absorptionMass SpectrometryJejunumIn vivoDepsipeptidesmedicineAnimalsIntestinal MucosaRats WistarGastrointestinal tractChromatographyStomachModels biològicsAnimal Feedmedicine.anatomical_structureBiochemistryIntestinal AbsorptionFermentationDuodenumFemaleChromatography Liquid
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Protective immunity against Echinostoma caproni in rats is induced by Syphacia muris infection.

2012

Syphacia muris (Nematoda: Oxyuridae) is a ubiquitous nematode that commonly infects rats in the laboratory and can interfere with the development of unrelated biological assays. In this context, we analysed the effect of a patent S. muris infection in Wistar rats on a superimposed infection with the intestinal trematode, Echinostoma caproni (Trematoda: Echinostomatidae). The results indicate that in the rats, infection with S. muris induces an immunity against a subsequent infection with E. caproni, although each parasite occupies different niches in the host. Echinostoma caproni worm recovery was significantly decreased in the rats primarily infected with S. muris and, at 3 and 4 weeks pos…

Antibodies HelminthIleumContext (language use)Trematode InfectionsImmunityIleumOxyuroideamedicineParasite hostingHelminthsAnimalsIntestinal MucosaRats WistarImmunity MucosalDisease ResistanceOxyuriasisEchinostomatidaebiologyMucinbiology.organism_classificationRatsDisease Models AnimalInfectious Diseasesmedicine.anatomical_structureNematodeImmunologyParasitologyFemaleTrematodaInternational journal for parasitology
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¿Se acercan los dos Foros?

2002

AntiglobalizaciónMundo justoVidal-Beneyto JoséParaísos fiscalesSociedad capitalistaDisentimientos políticosPoder políticoCrisisPublicaciones: Obra periodística: Columnas y artículos de opiniónUnión EuropeaEstablishmentGlobalizaciónMundo solidarioForo Mundial contra la PobrezaCorrupción políticaNueva YorkEnriquecimiento personalForo de Porto AlegrePOLÍTICAForo Social MundialDavosContestaciónFinanciación partidos políticosSOCIEDADLiberalismo multinacionalBeneficios millonariosBienestar
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Effect of nonprotein thiols on protein synthesis in isolated rat hepatocytes.

1996

The ability of nonprotein thiols to modulate rates of protein synthesis was investigated in isolated rat hepatocytes. Addition of cysteine stimulates protein labelling by [14C]Leucine. Glutathione depletion, induced by in vivo administration of L-buthionine sulfoximine and diethylmaleate, did not alter the effect of cysteine, although it decreased the rate of protein synthesis by 32%. The effect of cysteine on protein synthesis does not seem to be related to a perturbation of the redox state of the NAD+/NADH system or to changes in the rate of gluconeogenic pathway. The following observations indicate that cysteine may stimulate protein synthesis by increasing intracellular levels of aspart…

AntimetabolitesBiologyCellular and Molecular Neurosciencechemistry.chemical_compoundMethionineMethionine SulfoximineProtein biosynthesisAnimalsButhionine sulfoximineCarbon RadioisotopesCysteineSulfhydryl CompoundsAmino AcidsRats WistarMolecular BiologyButhionine SulfoximineCells CulturedPharmacologychemistry.chemical_classificationMaleatesAminooxyacetic AcidCell BiologyGlutathioneAmino acidRatsKineticsEnzymechemistryBiochemistryLiverProtein BiosynthesisMolecular MedicineNAD+ kinaseLeucineCysteineExperientia
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Glutathione metabolism in primary astrocyte cultures: flow cytometric evidence of heterogeneous distribution of GSH content.

1993

The time-course of intracellular glutathione (GSH) values after incubation with L-buthionine-(S,R)-sulfoximine (BSO), a selective inhibitor of gamma-glutamylcysteine synthetase, showed that glutathione turns over with a half-life of 5 h. Intracellular GSH was assayed by flow cytometry using three different methods. Astrocytes showed a narrow range of cellular size but a wide range of intracellular GSH. This heterogeneity was resolved into three distinct subpopulations which represent 20%, 35% and 45% of the total astrocyte number. The less abundant subpopulation had the lower GSH content, while the most abundant was the subpopulation with the higher content. Over 95% of astrocytes were in t…

AntimetabolitesNerve Tissue ProteinsBiologyFlow cytometrychemistry.chemical_compoundCytosolMethionine SulfoximinemedicineAnimalsButhionine sulfoximineRats WistarMolecular BiologyButhionine SulfoximineCells CulturedBrain ChemistryCerebral Cortexmedicine.diagnostic_testGeneral NeuroscienceCell CycleGlutathioneMetabolismDNAHydrogen-Ion ConcentrationFlow CytometryGlutathioneRatsCytosolmedicine.anatomical_structurechemistryBiochemistryAnimals NewbornAstrocytesNeurogliaNeurology (clinical)IntracellularDevelopmental BiologyAstrocyteHalf-LifeBrain research
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