Search results for "Disks"

showing 10 items of 118 documents

Involvement of cyclin-dependent kinase-5 in the kainic acid-mediated degeneration of glutamatergic synapses in the rat hippocampus.

2011

Increased levels of glutamate causing excitotoxic damage accompany neurological disorders such as ischemia/stroke, epilepsy and some neurodegenerative diseases. Cyclin-dependent kinase-5 (Cdk5) is important for synaptic plasticity and is deregulated in neurodegenerative diseases. However, the mechanisms by which kainic acid (KA)-induced excitotoxic damage involves Cdk5 in neuronal injury are not fully understood. In this work, we have thus studied involvement of Cdk5 in the KA-mediated degeneration of glutamatergic synapses in the rat hippocampus. KA induced degeneration of mossy fiber synapses and decreased glutamate receptor (GluR)6/7 and post-synaptic density protein 95 (PSD95) levels in…

MaleNeuronsKainic Acidhippocampuynaptic degenerationCalpainIntracellular Signaling Peptides and ProteinsMembrane ProteinsCyclin-Dependent Kinase 5Settore BIO/09 - FisiologiaHippocampusRatsReceptors Kainic AcidNerve DegenerationSynapsescyclin-dependent kinase-5Excitatory Amino Acid AgonistsAnimalsHumansCalciumRats WistarDisks Large Homolog 4 ProteinCells CulturedThe European journal of neuroscience
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Astronomiskās un dabas parādības aizvēsturē Ziemeļeiropā: atspoguļojums vēstures avotos un arheoloģiskajā materiālā

2021

Cilvēka dzīve aizvēsturē bija ļoti cieši saista ar dabu. Līdz ar pāreju uz ražotājsaimniecību vēlā akmens laikmeta beigās, bet īpaši sākot ar bronzas laikmetu, izveidojās ideoloģija, kurā centrālo vietu ieņēma Saule un ar to saistīto gadskārtu cikli. Solārā un lunārā simbolika plaši pārstāvēta Ziemeļeiropas, arī Latvijas arheoloģiskajā materiālā. Dabas un astronomiskās parādības minētas arī pirmajos rakstītajos avotos, bet to sekas – īpaši dabas katastrofu sekas, fiksējamas arī arheoloģiskajā materiālā.

Nebras debesu disks. Saksija Anhalte Vācija (1800 pr. Kr.)Virgas Kalnazīverti. 4.gs.Lielā 1264. gada komētaVikingu laikmets (793. – 1066.g.):HUMANITIES and RELIGION::History and philosophy subjects::History subjects::History [Research Subject Categories]Vēvelsburga (Wewelsburg) VācijaVilkumuižas ezersĀraišu ezerpils (9. – 10.gs.):HUMANITIES and RELIGION::History and philosophy subjects::Historical cultures::Classical archaeology and ancient history [Research Subject Categories]Septiņu sauļu (Siebenfältiges Sonnenwunder ) motīvsLielie Greizie ratiAlemāņu sakta. 7.gs.Ņūgrendža (Newgrange) Īrija (3200.g.pr. Kr.)Klimata izmaiņas bronzas laikmetāMazais ledus laikmetsSaules rati Trundholma Dānija (1400.pr. Kr.):HUMANITIES and RELIGION::History and philosophy subjects::Archaeology subjects::Archaeology [Research Subject Categories]
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GaInNAs/GaAs Bragg-mirror-based structures for novel 1.3μm device applications

2004

We report the use of GaInNAs/GaAs material system for a range of 1.3 μm vertical-cavity devices namely VCSELs, VCSOAs, VECSELs and SESAMs. Using optical pumping, we demonstrate that up to 4 mW of 1290 nm output power can be fibre-coupled from a VCSEL. We also show that tayloring the VCSEL structure allows to produce a monolithic long-wavelength VCSOA with up to 16 dB of gain. We also report the first demonstration of a 1.3 μm VECSEL with more than 0.5 W of CW ouptut power. Finally, annealing effects on the properties of a GaInNAs SBR and modelocking of two Nd:doped solid state lasers using this element are described.

Optical amplifierMaterials sciencePhotoluminescenceVideodisksbusiness.industryDopingSurface emitting lasersCondensed Matter PhysicsDistributed Bragg reflectorLaserSemiconductor laser theoryVertical-cavity surface-emitting laserlaw.inventionInorganic ChemistryOptical pumpingsemiconductor diskOpticslawMaterials ChemistryOptoelectronicsbusinessJournal of Crystal Growth
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Logopēda un vecāku sadarbības nozīme 3-4 gadu vecuma bērnu valodas un runas attīstības veicināšnā

2021

Darba tēma: Logopēda un vecāku sadarbības nozīme 3 – 4 gadu vecuma bērnu valodas un runas attīstības veicināšanā. Darba autore: Jekaterīna Kerevica Darba zinātniskā vadītāja: Lūcija Anoško Darbs sastāv no: 51 lpp., ievada, 5 nodaļām, teorētiskās daļas, praktiskās daļas, nobeiguma, secinājumiem, 3 tabulām, 17 attēli, 2 pielikumiem. Pētījuma mērķis: Teorētiski izzināt 3- 4 gadu vecuma posma bērna valodas un runas attīstību, praktiski pārbaudīt logopēda un vecāku kopīgās sadarbībās iespējas. Pētījuma priekšmets: Bērna valodas un runas attīstība 3 – 4 gadu vecumā. Teorētiskajā daļā darba autore, izmantojot analītisko metodi, padziļināti pētījusi zinātnisko literatūru par 3 - 4 gadu vecuma bērna…

PedagoģijaLogopēdu un vecāku sadarbībaLanguage and speechZīmējums kā metodisks līdzeklis.Cooperation between speech therapists and parentsValoda un runa
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Blue lasing at room temperature in high quality factor GaN/AlInN microdisks with InGaN quantum wells

2007

The authors report on the achievement of optically pumped III-V nitride blue microdisk lasers operating at room temperature. Controlled wet chemical etching of an AlInN interlayer lattice matched to GaN allows forming inverted cone pedestals. Whispering gallery modes are observed in the photoluminescence spectra of InGaN/GaN quantum wells embedded in the GaN microdisks. Typical quality factors of several thousands are found (Q>4000). Laser action at similar to 420 nm is achieved under pulsed excitation at room temperature for a peak power density of 400 kW/cm(2). The lasing emission linewidth is down to 0.033 nm.

PhotoluminescenceMaterials sciencePhysics and Astronomy (miscellaneous)business.industryBOXESSettore ING-INF/01 - ElettronicaSemiconductor laser theoryGANOptical pumpingMICROCAVITIESLaser linewidthOpticsLASERSSemiconductors Laser physics Photoluminescence spectroscopy Oscillator strengths Quantum wells Optical absorption Whispering gallery wave Nitrides Etching Electrical properties and parametersOptoelectronicsStimulated emissionWhispering-gallery waveGAAS MICRODISKSbusinessLasing thresholdQuantum well
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Discovery of 105 Hz coherent pulsations in the ultracompact binary IGR J16597-3704

2018

We report the discovery of X-ray pulsations at 105.2 Hz (9.5 ms) from the transient X-ray binary IGR J16597-3704 using NuSTAR and Swift. The source was discovered by INTEGRAL in the globular cluster NGC 6256 at a distance of 9.1 kpc. The X-ray pulsations show a clear Doppler modulation implying an orbital period of ~46 minutes and a projected semi-major axis of ~5 lt-ms, which makes IGR J16597-3704 an ultra-compact X-ray binary system. We estimated a minimum companion mass of 0.0065 solar masses, assuming a neutron star mass of 1.4 solar masses, and an inclination angle of <75 degrees (suggested by the absence of eclipses or dips in its light-curve). The broad-band energy spectrum of the…

PhotonAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencessymbols.namesakeAccretion accretion diskSettore FIS/05 - Astronomia E Astrofisica0103 physical sciencesBinaries: generalAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Accretion (meteorology)010308 nuclear & particles physicsgeneral; Stars: neutron; X-rays: binaries; Astronomy and Astrophysics; Space and Planetary Science [Accretion accretion disks; Binaries]Astronomy and AstrophysicsAstronomy and AstrophysicLight curveOrbital periodX-rays: binarieStars: neutronNeutron starSpace and Planetary ScienceGlobular clustersymbolsElectron temperatureAstrophysics - High Energy Astrophysical PhenomenaDoppler effect
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Reflection component in the Bright Atoll Source GX 9+9

2020

GX 9+9 (4U 1728-16) is a low mass X-ray binary (LMXB) source harboring a neutron star. Although it belongs to the subclass of the bright Atoll sources together with GX 9+1, GX 3+1, and GX 13+1, its broadband spectrum is poorly studied and apparently does not show reflection features in the spectrum. To constrain the continuum well and verify whether a relativistic smeared reflection component is present, we analyze the broadband spectrum of GX 9+9 using {\it BeppoSAX} and \textit{XMM-Newton} spectra covering the 0.3-40 keV energy band. We fit the spectrum adopting a model composed of a disk-blackbody plus a Comptonized component whose seed photons have a blackbody spectrum (Eastern Model). …

PhotonAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsColor temperature010502 geochemistry & geophysics01 natural sciencesSpectral lineX-rays: binariesstars: neutronAccretion accretion diskSettore FIS/05 - Astronomia E Astrofisicaaccretion0103 physical sciencesBlack-body radiation010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)accretion disksAstronomy and AstrophysicsX-rays: binarieAccretion (astrophysics)Neutron starSpace and Planetary ScienceElectron temperatureAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaLow Mass[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]stars: individual: GX 9+9
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Reconstruction of an Accretion Disk Image in AU Mon from CoRoT Photometry

2011

AbstractThe long-period binary system AU Mon was photometrically observed on-board the CoRoT satellite in a continuous run of almost 60 days long which has covered almost 5 complete cycles. Unprecedented sub milimag precision of CoRoT photometry reveals all complexity of its light variations in this, still active mass-transfer binary system. We present images of an accretion disk reconstructed by eclipse mapping, and an optimization of intensity distribution along disk surface. Time resolution and accurate CoRoT photometric measurements allow precise location of spatial distribution of ‘hot’ spots on the disk, and tracing temporal changes in their activity. Clumpy disk structure is similar …

Physics010308 nuclear & particles physicsBinary numberAstronomyAstronomy and AstrophysicsTime resolutionAstrophysicsSpatial distribution01 natural sciencesPhotometry (optics)accretion disks; eclipsing binaries; AU MonAccretion discSpace and Planetary Science0103 physical sciencesBinary system010303 astronomy & astrophysics
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GSC 07396-00759 = V4046 Sgr C[D]: A Wide-separation Companion to the Close T Tauri Binary System V4046 Sgr AB

2011

We explore the possibility that GSC 07396-00759 (spectral type M1e) is a widely separated (~2.82', or projected separation ~12,350 AU) companion to the "old" (age ~12 Myr) classical T Tauri binary system V4046 Sgr AB, as suggested by the proximity and similar space motions of the two systems. If the two systems are equidistant and coeval, then GSC 07396--00759, like V4046 Sgr AB, must be a spectroscopic binary with nearly equal-mass components, and V4046 Sgr must be at least ~8 Myr old. Analysis of a serendipitous Chandra X-ray gratings spectrum and light curve as well as XMM-Newton light curves and CCD spectra of GSC 07396-00759 obtained during long exposures targeting V4046 Sgr AB reveals…

Physics010308 nuclear & particles physicsBinary numberFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsLight curve01 natural sciencesSpectral lineT Tauri starSettore FIS/05 - Astronomia E Astrofisicabinaries: close circumstellar matter protoplanetary disks stars: pre-main sequenceAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Science0103 physical sciencesBinary systemCircular orbitCircumbinary planet010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)
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Impacts of fragmented accretion streams onto Classical T Tauri Stars: UV and X-ray emission lines

2016

Context. The accretion process in Classical T Tauri Stars (CTTSs) can be studied through the analysis of some UV and X-ray emission lines which trace hot gas flows and act as diagnostics of the post-shock downfalling plasma. In the UV band, where higher spectral resolution is available, these lines are characterized by rather complex profiles whose origin is still not clear. Aims. We investigate the origin of UV and X-ray emission at impact regions of density structured (fragmented) accretion streams.We study if and how the stream fragmentation and the resulting structure of the post-shock region determine the observed profiles of UV and X-ray emission lines. Methods. We model the impact of…

Physics010504 meteorology & atmospheric sciencesstars:pre-mainsequenceFOS: Physical sciencesAstronomy and AstrophysicsAstrophysicsPlasma01 natural sciencesAccretion (astrophysics)RedshiftT Tauri starSettore FIS/05 - Astronomia E AstrofisicaAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary Scienceaccretionaccretion disks0103 physical sciencesEmission spectrumSpectral resolutionMagnetohydrodynamics010303 astronomy & astrophysicsChromosphereSolar and Stellar Astrophysics (astro-ph.SR)0105 earth and related environmental sciences
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