Search results for "OBJECTS"

showing 10 items of 197 documents

The neural mechanisms of word order processing revisited: electrophysiological evidence from Japanese.

2008

We present two ERP studies on the processing of word order variations in Japanese, a language that is suited to shedding further light on the implications of word order freedom for neurocognitive approaches to sentence comprehension. Experiment 1 used auditory presentation and revealed that initial accusative objects elicit increased processing costs in comparison to initial subjects (in the form of a transient negativity) only when followed by a prosodic boundary. A similar effect was observed using visual presentation in Experiment 2, however only for accusative but not for dative objects. These results support a relational account of word order processing, in which the costs of comprehen…

AdultMaleLinguistics and LanguagePhraseCognitive NeuroscienceDative caseExperimental and Cognitive PsychologylinearizationLanguage and LinguisticsSpeech and HearingAsian PeopleSubject (grammar)P600HumansN400Argument (linguistics)Evoked PotentialsLanguageInformation processingBrainElectroencephalographyLinguisticsElectrophysiologyJapaneseSpeech PerceptionVisual PerceptionFemalePsychologySentenceWord orderCognitive psychologyInitial and terminal objectsBrain and language
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Developing motor planning over ages

2009

International audience; Few studies have explored the development of response selection processes in children in the case of object manipulation. In the current research, we studied the end-state comfort effect, the tendency to ensure a comfortable position at the end rather than at the beginning of simple object manipulation tasks. We used two versions of the unimanual bar transport task. In Experiment 1, only 10-year-olds reached the same level of sensitivity to end-state comfort as adults, and 8-year-olds were less efficient than 6-year-olds. In each age group, children’s sensitivity did not increase during a session: i.e., either clearly showed the sensitivity or showed no sensitivity a…

AdultMaleMotor developmenteducationExperimental and Cognitive PsychologyObjects and tools050105 experimental psychologySession (web analytics)Developmental psychologyTask (project management)03 medical and health sciencesChild Guidance0302 clinical medicinePrimary school childrenHand strengthTask Performance and AnalysisDevelopmental and Educational PsychologyCognitive developmentHumans0501 psychology and cognitive sciencesSensitivity (control systems)ChildMotor skillHand Strength05 social sciencesCognitionEnd-state comfort effectKindergartenersMotor SkillsChild Preschool[SCCO.PSYC]Cognitive science/PsychologyTask analysisFemalePsychologyPsychomotor Performance030217 neurology & neurosurgeryCognitive psychologyMotor planning
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BIM Modelling of Ancient Buildings

2018

In the last years, new procedures on design and management of constructions, based on 3D standardised models of building elements, have been proposed. It’s the case of Building Information Modelling (BIM) applications, that, differently from CAD ones, allow to work with libraries of 3D parametrical objects (smart objects) describing geometric, structural and material properties of building elements. This methodology is based on the Industry Foundation Classes (IFC) model, that represents a global standard for the building data exchange. Initially used for the design of new architectures, BIM methodology has been even more considered also for the management and the conservation of historical…

Architectural engineeringComputer scienceSmart objectsbusiness.industry0211 other engineering and technologies020101 civil engineering02 engineering and technology3D modelling0201 civil engineeringVariety (cybernetics)Cultural heritageLimit (category theory)Work (electrical)Building information modelingArchaeologyData exchangeHBIM021105 building & constructionIndustry Foundation ClassesCultural heritagebusinessSurveySettore ICAR/06 - Topografia E CartografiaGeospatial DB
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Being Opposite. On the translation of antikeimena in Aristotle's De anima

2012

The main concern of this article is the interpretation of De Anima II.4 415a14-23, and the particular way by which it is generally translated by modern editors. Almost all modern translations adopt the two locutions - \emph{objects} and \emph{correlative objects} - to translate the Greek word \antikeimena. But this choice is not neutral, nor it is without consequences for the understanding of the text.

Aristotle hylomorphism soul faculties objects perception intellect intentionalitySettore M-FIL/07 - Storia Della Filosofia AnticaSettore M-FIL/01 - Filosofia Teoretica
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A Flexible 4G/5G Control Platform for Fingerprint-based Indoor Localization

2019

In this paper we propose a centralized SDN platform devised to control indoor femto-cells for supporting multiple network-wide optimizations and applications. In particular, we focus on an example localization application in order to enlighten the main functionalities and potentialities of the approach. First, we demonstrate that the platform can be exploited for reconfiguring some operational procedures, based on standard signalling mechanisms, at the programmable femto-cells; these procedures enable customized logics for collecting measurements reports from mobile terminals. Second, assuming that high-density devices such as smart objects are disseminated in the controlled indoor space, w…

Artificial neural networkSmart objectsbusiness.industryComputer scienceReal-time computing020206 networking & telecommunications02 engineering and technologyBase stationSoftware0202 electrical engineering electronic engineering information engineeringCellular network020201 artificial intelligence & image processingbusinessClassifier (UML)5GIEEE INFOCOM 2019 - IEEE Conference on Computer Communications Workshops (INFOCOM WKSHPS)
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Oxygen depletion in dense molecular clouds: a clue to a low O2 abundance?

2011

Context: Dark cloud chemical models usually predict large amounts of O2, often above observational limits. Aims: We investigate the reason for this discrepancy from a theoretical point of view, inspired by the studies of Jenkins and Whittet on oxygen depletion. Methods: We use the gas-grain code Nautilus with an up-to-date gas-phase network to study the sensitivity of the molecular oxygen abundance to the oxygen elemental abundance. We use the rate coefficient for the reaction O + OH at 10 K recommended by the KIDA (KInetic Database for Astrochemistry) experts. Results: The updates of rate coefficients and branching ratios of the reactions of our gas-phase chemical network, especially N + C…

AstrochemistryChemical models[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Analytical chemistrychemistry.chemical_elementFOS: Physical sciencesAstrophysicsAstrophysicsKinetic energy01 natural sciencesOxygen[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]0103 physical sciencesSolar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysics010304 chemical physics[SDU.ASTR.SR]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]Molecular cloudAstronomy and Astrophysicsastrochemistry; ISM; abundances; ISM; molecules; ISM; individual objects; L134N; ISM; individual objects; TMC-1[PHYS.ASTR.SR]Physics [physics]/Astrophysics [astro-ph]/Solar and Stellar Astrophysics [astro-ph.SR]NitrogenchemistryAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceMolecular oxygenChemical network
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The hyperfine structure in the rotational spectrum of CF+

2012

Context. CF+ has recently been detected in the Horsehead and Orion Bar photo-dissociation regions. The J=1-0 line in the Horsehead is double-peaked in contrast to other millimeter lines. The origin of this double-peak profile may be kinematic or spectroscopic. Aims. We investigate the effect of hyperfine interactions due to the fluorine nucleus in CF+ on the rotational transitions. Methods. We compute the fluorine spin rotation constant of CF+ using high-level quantum chemical methods and determine the relative positions and intensities of each hyperfine component. This information is used to fit the theoretical hyperfine components to the observed CF+ line profiles, thereby employing the h…

AstrochemistryFOS: Physical sciencesContext (language use)Astrophysics010402 general chemistryRotation01 natural sciencesISM: clouds0103 physical sciencesSpin (physics)010303 astronomy & astrophysicsHyperfine structureAstrophysics::Galaxy AstrophysicsLine (formation)PhysicsNebularadio lines: ISMastrochemistryAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesISM: molecules0104 chemical sciences[PHYS.ASTR.GA]Physics [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Space and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)ISM: individual objects: Horsehead nebula[SDU.ASTR.GA]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Galactic Astrophysics [astro-ph.GA]Atomic physicsBar (unit)
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Absolute kinematics of radio-source components in the complete S5 polar cap sample: IV. Proper motions of the radio cores over a decade and spectral …

2016

We have carried out a high-precision astrometric analysis of two very-long-baseline-interferometry (VLBI) epochs of observation of the 13 extragalactic radio sources in the complete S5 polar cap sample. The VLBI epochs span a time baseline of ten years and enable us to achieve precisions in the proper motions of the source cores up to a few micro-arcseconds per year. The observations were performed at 14.4 GHz and 43.1 GHz, and enable us to estimate the frequency core-shifts in a subset of sources, for which the spectral-index distributions can be computed. We study the source-position stability by analysing the changes in the relative positions of fiducial source points (the jet cores) ove…

AstrofísicaActive galactic nucleusAstrometriaAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsKinematics01 natural sciencesStability (probability)Radio continuum: generalBinary black hole0103 physical sciencesVery-long-baseline interferometry010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsJet (fluid)general [Radio continuum]general [BL Lacertae objects]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicsgeneral [Quasars]BL Lacertae objects: generalAstrometryAstrometryAstrophysics - Astrophysics of GalaxiesQuasars: generalGravitational lensSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Techniques: interferometricinterferometric [Techniques]Astrophysics - Instrumentation and Methods for Astrophysics
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EVIDENCE OF NON-THERMAL X-RAY EMISSION FROM HH 80

2013

Protostellar jets appear at all stages of star formation when the accretion process is still at work. Jets travel at velocities of hundreds of km s -1, creating strong shocks when interacting with the interstellar medium. Several cases of jets have been detected in X-rays, typically showing soft emission. For the first time, we report evidence of hard X-ray emission possibly related to non-thermal processes not explained by previous models of the post-shock emission predicted in the jet/ambient interaction scenario. HH 80 is located at the south head of the jet associated with the massive protostar IRAS 18162-2048. It shows soft and hard X-ray emission in regions that are spatially separate…

AstrofísicaCiencias AstronómicasCiencias FísicasAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesSynchrotron radiationAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsIndividual: Iras 18162-2048 [Stars]//purl.org/becyt/ford/1 [https]Herbig-Haro objects ISM: jets and outflows radiation mechanisms: non-thermal stars: individual: IRAS 18162-2048 stars: pre-main sequence X-rays: generalHigh Energy Physics - Phenomenology (hep-ph)Herbig-Haro objectsGeneral [X-Rays]jets and outflows radiation mechanisms: non-thermal stars: individual: IRAS 18162-2048 stars: pre-main sequence X-rays: general [Herbig-Haro objects ISM]Jets And Outflows [Ism]ThermalProtostarstars: individualAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsStar formationX-rayAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]radiation mechanisms: non-thermalHerbig-Haro ObjectsAstrophysics - Astrophysics of GalaxiesAccretion (astrophysics)Non-Thermal [Radiation Mechanisms]AstronomíaInterstellar mediumHigh Energy Physics - PhenomenologyISM: jets and outflowsSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics - High Energy Astrophysical PhenomenaCIENCIAS NATURALES Y EXACTASThe Astrophysical Journal
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X-ray emission from stellar jets by collision against high-density molecular clouds: an application to HH 248

2015

We investigate the plausibility of detecting X-ray emission from a stellar jet that impacts against a dense molecular cloud. This scenario may be usual for classical T Tauri stars with jets in dense star-forming complexes. We first model the impact of a jet against a dense cloud by 2D axisymmetric hydrodynamic simulations, exploring different configurations of the ambient environment. Then, we compare our results with XMM-Newton observations of the Herbig-Haro object HH 248, where extended X-ray emission aligned with the optical knots is detected at the edge of the nearby IC 434 cloud. Our simulations show that a jet can produce plasma with temperatures up to 10 MK, consistent with producti…

AstrofísicaHERBIGHARO OBJECTSJETS AND OUTFLOWS [ISM]Astrophysics::High Energy Astrophysical PhenomenaRotational symmetryFOS: Physical sciencesCloud computingAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsISM [X-RAYS]Space (mathematics)LuminosityHYDRODYNAMICS//purl.org/becyt/ford/1 [https]INDIVIDUAL OBJECTS (HH 248) [ISM]hydrodynamics Herbig-Haro objects ISM: individual objects: HH 248 ISM: jets and outflows X-rays: ISMAstrophysics::Galaxy AstrophysicsSolar and Stellar Astrophysics (astro-ph.SR)PhysicsJet (fluid)business.industryMolecular cloudAstronomy and Astrophysics//purl.org/becyt/ford/1.3 [https]PlasmaAstronomíaT Tauri starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceHerbig–Haro objectsbusiness
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