Search results for " star"

showing 10 items of 1194 documents

Multimodal Assessment of Long-Term Memory Recall and Reinstatement in a Combined Cue and Context Fear Conditioning and Extinction Paradigm in Humans

2013

Learning to predict danger via associative learning processes is critical for adaptive behaviour. After successful extinction, persisting fear memories often emerge as returning fear. Investigation of return of fear phenomena, e.g. reinstatement, have only recently began and to date, many critical questions with respect to reinstatement in human populations remain unresolved. Few studies have separated experimental phases in time even though increasing evidence shows that allowing for passage of time (and consolidation) between experimental phases has a major impact on the results. In addition, studies have relied on a single psychophysiological dimension only (SCRs/SCL or FPS) which hamper…

AdultReflex StartleMemory Long-TermConditioning Classicallcsh:MedicineContext (language use)Neuropsychological TestsBiologyExtinction PsychologicalArousalHumansFear conditioninglcsh:ScienceCued speechMultidisciplinaryRecallLong-term memorylcsh:RAssociation LearningFearGalvanic Skin ResponseExtinction (psychology)Middle AgedAssociative learninglcsh:QCuesArousalResearch ArticleCognitive psychologyPLoS ONE
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Speeding up gait initiation and gait-pattern with a startling stimulus.

2008

Human gait involves a repetitive leg motor pattern that emerges after gait initiation. While the automatic maintenance of the gait-pattern may be under the control of subcortical motor centres, gait initiation requires the voluntary launching of a different motor program. In this study, we sought to examine how the two motor programmes respond to an experimental manipulation of the timing of gait initiation. Subjects were instructed to start walking as soon as possible at the perception of an imperative signal (IS) that, in some interspersed trials was accompanied by a startling auditory stimulus (SAS). This method is known to shorten the latency for execution of the motor task under prepar…

Adultmedicine.medical_specialtyReflex StartleTime Factorsmedia_common.quotation_subjectAccelerationPostureBiophysicsMotor programStimulus (physiology)Physical medicine and rehabilitationGait (human)PerceptionmedicineHumansOrthopedics and Sports MedicineGait initiationMuscle SkeletalGaitmedia_commonAnalysis of VarianceLegElectromyographyRehabilitationCentral pattern generatorMiddle AgedMotor taskAcoustic StimulationPhysical therapyGait patternPsychologyhuman activitiesPhotic StimulationGaitposture
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"Piosenka jest dobra na wszystko" : propozycja bloku zajęć zapoznających studentów obcojęzycznych z wybranymi utworami twórców polskiej piosenki

2022

Artykuł stanowi omówienie propozycji bloku zajęć adresowanych do studentów obcojęzycznych, którego celem jest wzmocnienie kompetencji językowych, ale także przybliżenie sylwetek kilku znaczących reprezentantów polskiej sceny muzycznej: Czesława Niemena, Agnieszki Osieckiej, Wojciecha Młynarskiego, Kabaretu Starszych Panów. W założeniu ma to służyć podniesieniu motywacji cudzoziemców do nauki języka polskiego. Zaproponowane zajęcia są adresowane do studentów posługujących się językiem polskim co najmniej na poziomie B1+/B2, jednak - biorąc pod uwagę - holistyczne podejście do nauczania języka obcego, można na ich podstawie skonstruować serię zadań doskonalących różnorakie kompetencje językow…

Agnieszka Osieckapiosenka w nauczaniu języka polskiego jako obcegoCzesław Niemenkultura w nauczaniu języka polskiego jako obcegoKabaret Starszych Panówsong in teaching Polish as a foreign languageWojciech Młynarskiculture in teaching Polish as a foreign language
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Optical and ultraviolet pulsed emission from an accreting millisecond pulsar

2021

Ambrosino, F., et al.

Angular momentum010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaMagnetosphereFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesLuminosityNeutron starsSettore FIS/05 - Astronomia E AstrofisicaPulsarMillisecond pulsar0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astronomy and AstrophysicsAccretion (astrophysics)Particle accelerationNeutron starAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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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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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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Figures of equilibrium in close binary systems

1992

The equilibrium configurations of close binary systems are analyzed. The autogravitational, centrifugal and tidal potentials are expanded in Clairaut's coordinates. From the set of the total potential angular terms an integral equations system is derived. The reduction of them to ordinary differential equations and the determination of the boundary conditions allow a formulation of the problem in terms of a single variable.

Applied MathematicsMathematical analysisfigure of celestial bodiesspherical harmonicsBinary numberSpherical harmonicsAstronomy and AstrophysicsIntegral equationCelestial mechanicsComputational MathematicsClassical mechanicsSpace and Planetary ScienceModeling and SimulationOrdinary differential equationPoisson equationsclose binary starsBoundary value problemPoisson's equationReduction (mathematics)Mathematical PhysicsMathematicsCelestial Mechanics and Dynamical Astronomy
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Influence of Physical Treatments on the Potato Starch Granules Micro- and Ultrastructure

2012

In this research, potato starch was subjected to ph ysical treatments in order to analyse the changes at the micro- and ultrastructural levels an d finally to identify the optimal conditions for disintegrating the starch granules. For the analysi s, 10% aqueous solutions of potato starch were treated with a) microwaves; b) heat and c) heat com bined with ultrasounds. For each treatment type, the duration was 5 minutes, excepting the microwave treatment, where the time was 1 and 5 minutes; heat power varied from 180W to 900W at the tests with microwave, temperature varied between 65 o C and 100 o C in the thermal experiments and at the thermal ana lysis combined with ultrasounds temperature …

Aqueous solutionLysisStarchGeography Planning and DevelopmentGranule (cell biology)Thermal treatmentManagement Monitoring Policy and LawMicrostructurechemistry.chemical_compoundchemistryBotanyUltrastructurePotato starchNuclear chemistryBulletin of University of Agricultural Sciences and Veterinary Medicine Cluj-Napoca. Agriculture
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