Search results for "Star"

showing 10 items of 4285 documents

Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO-Virgo Run O3a

2022

Abbott, R., et al. (LIGO and VIRGO Collaboration)

neutron star: binaryGravitational waves(678)ELECTROMAGNETIC COUNTERPARTSBinary numberAstrophysics01 natural sciencesLIGOHigh-Energy Phenomena and Fundamental PhysicsQCSUPERNOVAQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Settore FIS/01education.field_of_study[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Black holesSettore FIS/0506 humanities and the artsGRBEnergy InjectionSearch for gravitational wave transients associated to GRBs - Fermi and Swift satellitesAFTERGLOWPhysical SciencesRELATIVISTIC JETSAstrophysics - High Energy Astrophysical PhenomenaSwiftGravitational waveBlack-Hole330Evolutiongr-qcGamma Ray Burst LIGO Virgo Gravitational WavesAstrophysics::High Energy Astrophysical PhenomenaGeneral Relativity and Quantum Cosmology (gr-qc)0603 philosophy ethics and religionGravitational-wave astronomyNeutron starsENERGY INJECTIONCORE-COLLAPSEeducationGamma-ray burstScience & TechnologyCore-CollapseVirgoRCUKAstronomy and AstrophysicstriggerLuminosity FunctionDewey Decimal Classification::500 | Naturwissenschaften::520 | Astronomie KartographieGamma Ray BurstSpace and Planetary ScienceBLACK-HOLEddc:520gravitational wave astronomyGravitational wave astronomyGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]LIGO(920)Fermi Gamma-ray Space TelescopeAstronomyAstrophysicsGeneral Relativity and Quantum Cosmologyneutron starsENERGYGravitational wave detectorsGamma-ray bursts(629)Neutron Stars Mergers Gravitational Waves010303 astronomy & astrophysicsgravitational waves; gamma ray bursts; LIGO; Virgo; Fermi; SwiftCompact binary stars(283)astro-ph.HEPhysicscompact binary starsgamma-ray burstsgamma-ray bursts ; gravitational waves; LIGO; Virgogravitational waves060302 philosophy[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]PRECURSOR ACTIVITYGravitational wave astronomy(675)Gamma-ray burstsGW_HIGHLIGHT[PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE]PopulationCompact binary starssatelliteFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstronomy & Astrophysicsgamma ray: burstMASS1STGLASTGamma-ray bursts; Gravitational wave astronomy; Gravitational waves; Gravitational wave detectors0103 physical sciencesSTFCFermigravitational waves; gamma-ray bursts; LIGO; Virgo; Fermi; SwiftGravitational wavegravitational radiationgamma ray burstsgamma-ray burts--black holesLIGOEVOLUTIONOBSERVING RUNNeutron stars(1108)Neutron starPhysics and Astronomy[SDU]Sciences of the Universe [physics]LUMINOSITY FUNCTIONBlack holes(162)INJECTIONEMISSION
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The advanced Virgo longitudinal control system for the O2 observing run

2020

Following a successful period of data-taking between 2006 and 2011, the Virgo gravitational-wave detector was taken offline for a major upgrade. The changes made to the instrument significantly increased the complexity of the control systems and meant that an extended period of commissioning was required to reach a sensitivity appropriate for science data-taking. This commissioning period was completed in July of 2017 and the second-generation Advanced Virgo detector went on to join the Advanced LIGO detectors in the O2 science run in August of the same year. The upgraded detector was approximately twice as sensitive to binary neutron star mergers as the first-generation instrument. During …

neutron star: binaryPhysics::Instrumentation and DetectorsAstronomycavity: opticalSuspended optical cavities01 natural sciencesGravitational wave detectorsoff-lineGravitational wave detectors; Interferometer; Suspended optical cavities; Control loopsControl loopSuspended optical cavitieLIGOInterferometer010303 astronomy & astrophysicsdetectorsSettore FIS/01Physics[PHYS]Physics [physics]DetectorAstrophysics::Instrumentation and Methods for AstrophysicsGravitational wave detectors Interferometer Suspended optical cavities Control loopsGravitational wave detectorUpgrade[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]upgradecontrol systemGravitational wavelongitudinalAstrophysics::High Energy Astrophysical PhenomenainterferometerAstrophysics::Cosmology and Extragalactic Astrophysicscontrol loops; gravitational wave detectors; interferometer; suspended optical cavitiesgravitational radiation: direct detectionGeneral Relativity and Quantum CosmologySettore FIS/05 - Astronomia e AstrofisicaBinary black holebinary: coalescence0103 physical sciencesControl loops[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]010308 nuclear & particles physicsGravitational wavegravitational radiationAstronomyAstronomy and AstrophysicssensitivityLIGOgravitational radiation detectordetector: sensitivityNeutron star* Automatic Keywords *VIRGOblack hole: binaryControl systemgravitational radiation: emission[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

2017

On August 17, 2017 at 12-41:04 UTC the Advanced LIGO and Advanced Virgo gravitational-wave detectors made their first observation of a binary neutron star inspiral. The signal, GW170817, was detected with a combined signal-to-noise ratio of 32.4 and a false-alarm-rate estimate of less than one per 8.0×104 years. We infer the component masses of the binary to be between 0.86 and 2.26 M, in agreement with masses of known neutron stars. Restricting the component spins to the range inferred in binary neutron stars, we find the component masses to be in the range 1.17-1.60 M, with the total mass of the system 2.74-0.01+0.04M. The source was localized within a sky region of 28 deg2 (90% probabili…

neutron star: binary[ PHYS.ASTR ] Physics [physics]/Astrophysics [astro-ph]X-ray binaryADVANCED LIGOAstrophysicsKilonovagravitational waves; LIGO; binary neutron star inspiralspin01 natural sciencesLIGOGeneralLiterature_REFERENCE(e.g.dictionariesencyclopediasglossaries)QCQBHigh Energy Astrophysical Phenomena (astro-ph.HE)Electromagnetic observationsGravitational-wave signals3100 General Physics and AstronomyPoint MassesAstrophysics - High Energy Astrophysical PhenomenaBlack-Hole MergersBinary neutron starsBlack HolesX-ray bursterCoalescing BinariesAstrophysics::High Energy Astrophysical Phenomena10192 Physics InstituteGeneral Relativity and Quantum Cosmology (gr-qc)Gravity wavesGravitational wavesNeutron starsPhysics and Astronomy (all)ddc:530Electromagnetic spectraNeutrons010308 nuclear & particles physicsVirgoGamma raysAstronomyRCUKVIRGOelectromagneticgravitational radiation: emissionStellar black holeGamma-ray burst[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Compact Binariesbinary: masscosmological modelAstronomyGeneral Physics and AstronomyAstrophysicsneutron starsGamma ray burstsGeneral Relativity and Quantum CosmologyGravitational wave detectorsUniverseDENSE MATTER010303 astronomy & astrophysicsastro-ph.HEPhysicsSignal to noise ratioSettore FIS/01 - Fisica SperimentaleGravitational effectsFalse alarm rateEQUATION-OF-STATEMergers and acquisitionsgravitational waves[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]530 PhysicsMERGERSGeneral Relativity and Quantum Cosmology; General Relativity and Quantum Cosmology; astro-ph.HEFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic Astrophysicsgamma ray: burstgravitational radiation: direct detectionMerging[ PHYS.GRQC ] Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]GAMMA-RAY BURSTLIGO (Observatory)binary: coalescenceGravitational waves neutron stars gamma-ray burst LIGO Virgo0103 physical sciencesGW151226MASSESSTFCAstrophysics::Galaxy AstrophysicsPhysiqueGravitational wavegravitational radiationPULSARgravitational radiation detectorNeutron starPhysics and AstronomygravitationRADIATIONDewey Decimal Classification::500 | Naturwissenschaften::530 | Physikbinary neutron star inspiralSignal detectionPHYS REV LETT PHYSICAL REVIEW LETTERS
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New orbital ephemerides for the dipping source 4U 1323-619: Constraining the distance to the source

2016

4U 1323-619 is a low mass X-ray binary system that shows type I X-ray bursts and dips. The most accurate estimation of the orbital period is 2.941923(36) hrs and a distance from the source that is lower than 11 kpc has been proposed. We aim to obtain the orbital ephemeris, the orbital period of the system, as well as its derivative to compare the observed luminosity with that predicted by the theory of secular evolution. We took the advantage of about 26 years of X-ray data and grouped the selected observations when close in time. We folded the light curves and used the timing technique, obtaining 12 dip arrival times. We fit the delays of the dip arrival times both with a linear and a quad…

neutron X-rays: binaries X-rays: stars ephemerides stars: individual: 4U 1323-619 [stars]010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesContext (language use)AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsEphemeris01 natural sciencesLuminositySettore FIS/05 - Astronomia E Astrofisica0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)stars: neutron X-rays: binaries X-rays: stars ephemerides stars: individual: 4U 1323-619Astronomy and AstrophysicsLight curveOrbital periodGalaxyNeutron starSpace and Planetary ScienceAstrophysics::Earth and Planetary AstrophysicsLow MassAstrophysics - High Energy Astrophysical Phenomena
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Timing an Accreting Millisecond Pulsar: Measuring the Accretion Torque in IGR J00291+5934

2006

We performed a timing analysis of the fastest accreting millisecond pulsar IGR J00291+5934 using RXTE data taken during the outburst of December 2004. We corrected the arrival times of all the events for the orbital (Doppler) effects and performed a timing analysis of the resulting phase delays. In this way we have the possibility to study, for the first time in this class of sources, the spin-up of a millisecond pulsar as a consequence of accretion torques during the X-ray outburst. The accretion torque gives us for the first time an independent estimate of the mass accretion rate onto the neutron star, which can be compared with the observed X-ray luminosity. We also report a revised valu…

neutron; stars : magnetic fields; pulsars : general; pulsars : individual : IGR J00291+5934; X-ray : binaries [accretion accretion disks; stars]X-rays : binariesAstrophysics::High Energy Astrophysical PhenomenaX-ray binaryFOS: Physical sciencesAstrophysicsaccretion accretion diskAstrophysicsX-ray : binariesBinary pulsarLuminositypulsars : individual : IGR J00291+5934symbols.namesakePulsarMillisecond pulsarAstrophysics::Solar and Stellar Astrophysicspulsars : individual (IGR J00291+5934)PhysicsAccretion (meteorology)general; pulsars : individual (IGR J00291+5934); stars : magnetic fields; stars : neutron; X-rays : binaries [pulsars]Astrophysics (astro-ph)pulsars : generalStatic timing analysisAstronomystars : magnetic fieldAstronomy and Astrophysicsstars : neutronNeutron starSpace and Planetary SciencesymbolsAstrophysics::Earth and Planetary AstrophysicsDoppler effectX-ray pulsar
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Inference of proto-neutron star properties from gravitational-wave data in core-collapse supernovae

2021

The eventual detection of gravitational waves from core-collapse supernovae (CCSN) will help improve our current understanding of the explosion mechanism of massive stars. The stochastic nature of the late post-bounce gravitational wave signal due to the non-linear dynamics of the matter involved and the large number of degrees of freedom of the phenomenon make the source parameter inference problem very challenging. In this paper we take a step towards that goal and present a parameter estimation approach which is based on the gravitational waves associated with oscillations of proto-neutron stars (PNS). Numerical simulations of CCSN have shown that buoyancy-driven g-modes are responsible …

noiseGravitational-wave observatorygravitational radiation: stochasticAstrophysics::High Energy Astrophysical Phenomenaprotoneutron starDegrees of freedom (physics and chemistry)FOS: Physical sciencesAstrophysicsGeneral Relativity and Quantum Cosmology (gr-qc)01 natural sciences7. Clean energyGeneral Relativity and Quantum CosmologyEinstein Telescopeeffect: nonlinearsupernova0103 physical sciences[PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det]LIGOnumerical calculations010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)equation of statePhysicsSolar massmass: solarEinstein Telescope010308 nuclear & particles physicsGravitational wavegravitational radiationoscillationgravitational radiation detectorLIGOgravitation: collapsedetector: sensitivitystar: massiveSupernovaStarswave: modelVIRGO13. Climate actiongravitational radiation: emission[PHYS.GRQC]Physics [physics]/General Relativity and Quantum Cosmology [gr-qc]galaxyAstrophysics - Instrumentation and Methods for AstrophysicsAstrophysics and astroparticle physics
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Šķīrējtiesas nolēmumu apstrīdēšanas institūts starptautiskajā praksē

2015

Šķīrējtiesa ir pasaulē iecienītākais komercstrīdu izšķiršanas veids. Lai šķīrējtiesas institūts atbilstu mūsdienu komercvidei, gan starptautiskie, gan nacionālie šķīrējtiesas procesu regulējošie normatīvie akti tiek mainīti, modernizēti un pielāgoti jaunajiem apstākļiem. Šodien svarīgs šķīrējtiesas procesa elements ir šķīŗējtiesas nolēmuma tiesiskuma un taisnīguma uzraudzība, kuru var īstenot valsts institūcija izskatot pieteikumus par šķīrējtiesas nolēmuma atcelšanu. Latvijā, atšķirībā no citu pasaules valstu tiesību sistēmām, normas, kuras regulē šķīrējtiesas nolēmuma atcelšanu, ilgstoši nav grozītas. Jaunā Šķīrējtiesu likuma normas nesaskan ar starptautisko šķīrējtiesas nolēmumu atcelšan…

nolēmuma atcelšanas sekasnolēmuma atcelšanašķīrējtiesastarptautiskskomercstrīdiJuridiskā zinātne
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Ēšanas traucējumu saistība ar starppersonu uzvedības efektivitāti

2019

Pētījuma mērķis bija noskaidrot pastāvošās sakarības starp ēšanas traucējumu simptomu izteiktību un personas funkcionēšanu starppersonu attiecībās, tādējādi papildinot Latvijā veikto ēšanas traucējumu jomas izpēti ar iepriekš neskartu tēmu. Tika aptaujātas 72 sievietes vecumā no 18 gadiem, bet 2 vecāko dalībnieču rezultāti izslēgti no pētījuma, jo tās katra bija vienīgā pārstāve savā vecuma grupā, 50-54 un 55-60 gadi; tādējādi dati apkopoti par 70 dalībniecēm vecumā no 18 līdz 50 gadiem. Pētījumā tika izmantotas divas aptaujas: Ēšanas traucējumu noteikšanas aptauja (Eating Disorder Examination Questionnaire EDE-Q 6.0, Fairburn & Beglin, 1994), ko Latvijā adaptējusi Ginta Jansone maģistra da…

norūpēšanās attiecībā uz ēdienuēšanas traucējuminorūpēšanās par ķermeņa svarustarppersonu efektivitātePsiholoģijanorūpēšanās par ķermeņa formu
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Noziedzīgi iegūtas mantas atgūšanas problemātika

2016

Noziedzīgi iegūtas mantas atgūšana ir vairāku savstarpēji saistītu procesu kopums, kā rezultātā noziedzīgi iegūta manta tiek konfiscēta vai atgriezta likumīgajam īpašniekam. Atgūšanas procesi ir: noziedzīgi iegūtās mantas identificēšana, arests, pierādījumu iegūšana mantas noziedzīgajai izcelsmei, kas ietver arī starptautisko sadarbību, un galējā nolēmuma par mantu pieņemšana. Veiksmīgai noziedzīgi iegūtas mantas atgūšanai nepieciešama visu iepriekš minēto procesu nekļūdīga norise un valsts ieinteresētība izveidot tādus politikas plānošanas dokumentus un tiesisko regulējumu, lai uzlabotu noziedzīgi iegūtas mantas atgūšanas procesus. Pētījuma mērķis bija izpētīt noziedzīgi iegūtas mantas atg…

noziedzīgi iegūta mantaaresta uzlikšana mantaimantas noziedzīgās izcelsmes prezumēšanaarestētās mantas saglabāšanastarptautiskā sadarbība līdzekļu atgūšanas jomāJuridiskā zinātne
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Starplēmuma un administratīvā akta nošķiršanas problemātika

2020

Starplēmuma un administratīvā akta nošķiršanas nozīmīgumu var pamatot ar faktu, ka starplēmums nav pārsūdzams atsevišķi no administratīvā akta. Bakalaura darba mērķis ir izpētīt un analizēt būtiskākās atšķirības starp starplēmumu un administratīvo aktu, kā arī noskaidrot tiesu praksē pastāvošo nošķiršanas problemātiku un nošķiršanas dažādību. Darba uzdevumi ir apzināt gadījumus, kad starplēmums ir un kad nav uzskatāms par administratīvo aktu, noskaidrot starplēmuma apstrīdēšanas un pārsūdzības iespējas atsevišķi no administratīvā akta un izpētīt sūdzības kārtības institūtu. Bakalaura darba rezultātā autore secina, ka tiesu praksē pastāv neviennozīmīga izpratne par atsevišķu lēmumu tiesisko …

nošķiršanastarplēmumsadministratīvais aktsstarplēmums ar būtisku ietekmiJuridiskā zinātne
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