Search results for "STARS"

showing 8 items of 798 documents

Non-stationary dynamo and magnetospheric accretion processes of the classical T Tauri star V2129 Oph

2011

We report here the first results of a multiwavelength campaign focussing on magnetospheric accretion processes of the classical T Tauri star V2129 Oph. In this paper, we present spectropolarimetric observations collected in 2009 July with ESPaDOnS at the Canada-France-Hawaii Telescope and contemporaneous photometry secured with the SMARTS facility. Circularly polarized Zeeman signatures are clearly detected, both in photospheric absorption and accretion-powered emission lines, from time-series of which we reconstruct new maps of the magnetic field, photospheric brightness and accretion-powered emission at the surface of V2129 Oph using our newest tomographic imaging tool - to be compared wi…

techniques: polarimetric stars: formation stars: imaging stars: individual: V2129 Oph stars: magnetic field stars: rotationSettore FIS/05 - Astronomia E Astrofisica
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Chandra study of the eclipsing M dwarf binary, YY Gem

2012

The eclipsing M dwarf binary system, YY Gem, was observed using Chandra covering 140 ks (2Prot) in total, split into two even exposures separated by 0.76 d (0.94 Prot). The system was extremely active: three energetic flares were observed over the course of these observations. The flaring and non-flaring states of the system are analysed in this paper. The activity level increased between the first and second observations even during the quiescent (non-flaring) phases. An analysis of the dynamics of the X-ray-emitting plasma suggests that both components are significantly active. Contemporaneous Hα spectra also suggest that both components show similar levels of activity. The primary star i…

techniques: spectroscopic binaries: eclipsing stars: coronae stars: flare stars: magnetic field X-rays: starsspectroscopic binaries: eclipsing stars: coronae stars: flare stars: magnetic field X-rays: stars [techniques]Settore FIS/05 - Astronomia E Astrofisica
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Osoba starsza w perspektywie systemowej terapii rodzin

2015

terapia systemowa rodzinyosoba starsza
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Three-dimensional core-collapse supernovae with complex magnetic structures: I. Explosion dynamics

2021

Magnetic fields can play a major role in the dynamics of outstanding explosions associated to violent events such as GRBs and hypernovae, since they provide a natural mechanism to harness the rotational energy of the central proto-neutron star and power relativistic jets through the stellar progenitor. As the structure of such fields is quite uncertain, most numerical models of MHD-driven core-collapse supernovae consider an aligned dipole as initial magnetic field, while the field's morphology can actually be much more complex. We present three-dimensional simulations of core-collapse supernovae with more realistic magnetic structures, such as quadrupolar fields and, for the first time, an…

transients: supernovaeField (physics)MHDAstrophysics::High Energy Astrophysical Phenomenagamma-ray burst: generalFOS: Physical sciencesAstrophysics01 natural sciencesstars: magnetarsAstrophysical jet0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)relativistic processesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsRotational energyMagnetic fieldDipoleAstrophysics - Solar and Stellar AstrophysicsinstabilitiesSpace and Planetary ScienceMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]HypernovaDynamo
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The impact of non-dipolar magnetic fields in core-collapse supernovae

2019

The magnetic field is believed to play an important role in at least some core-collapse supernovae if its magnitude reaches $10^{15}\,\rm{G}$, which is a typical value for a magnetar. In the presence of fast rotation, such a strong magnetic field can drive powerful jet-like explosions if it has the large-scale coherence of a dipole. The topology of the magnetic field is, however, probably much more complex with strong multipolar and small-scale components and the consequences for the explosion are so far unclear. We investigate the effects of the magnetic field topology on the dynamics of core-collapse supernovae and the properties of forming proto-neutron star (PNS) by comparing pre-collap…

transients: supernovaeMHDAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesCompact starMagnetar01 natural sciencesstars: magnetars0103 physical sciences010303 astronomy & astrophysicsrelativistic processesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Toroid010308 nuclear & particles physicsgamma-ray burststurbulenceAstronomy and AstrophysicsRotational energyComputational physicsMagnetic fieldSupernovaDipoleSpace and Planetary ScienceMagnetohydrodynamicsAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Monthly Notices of the Royal Astronomical Society
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Aktywizacja seniorów na przykładzie działalności edukacyjnej i kulturalno-społecznej Uniwersytetu Trzeciego Wieku w Kędzierzynie-Koźlu

2022

wykluczenie społeczneUniwersytet Trzeciego Wiekusocial exclusionaktywizacja seniorówactivation of seniorsdziałalność kulturalno-społecznaeducation of older peoplecultural and social activitiesKędzierzyn-KoźleUniversity of the Third Ageedukacja osób starszych
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The Large Observatory For x-ray Timing

2014

The Large Observatory For x-ray Timing (LOFT) was studied within ESA M3 Cosmic Vision framework and participated in the final down-selection for a launch slot in 2022-2024. Thanks to the unprecedented combination of effective area and spectral resolution of its main instrument, LOFT will study the behaviour of matter under extreme conditions, such as the strong gravitational field in the innermost regions of accretion flows close to black holes and neutron stars, and the supra-nuclear densities in the interior of neutron stars. The science payload is based on a Large Area Detector (LAD, 10 m 2 effective area, 2-30 keV, 240 eV spectral resolution, 1 deg collimated field of view) and a WideFi…

x-ray and γ-ray instrumentationcompact objects; microchannel plates; X-ray detectors; X-ray imaging; X-ray spectroscopy; X-ray timing; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Computer Science Applications1707 Computer Vision and Pattern Recognition; Applied Mathematics; Electrical and Electronic EngineeringVisionX-ray timingObservatoriesField of view01 natural sciences7. Clean energyneutron starsObservatory010303 astronomy & astrophysicsPhysicsEquipment and servicesApplied MathematicsAstrophysics::Instrumentation and Methods for AstrophysicsSteradian[ SDU.ASTR.IM ] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Computer Science Applications1707 Computer Vision and Pattern RecognitionX-ray detectorsCondensed Matter Physicscompact objectsX-ray spectroscopyAstrophysics - Instrumentation and Methods for AstrophysicsX-ray detector[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Cosmic VisionSpectral resolutionmicrochannel platesAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesNOmicrochannel platecompact objects; microchannel plates; X-ray detectors; X-ray imaging; X-ray spectroscopy; X-ray timing; Electronic Optical and Magnetic Materials; Condensed Matter Physics; Applied Mathematics; Electrical and Electronic EngineeringSettore FIS/05 - Astronomia e AstrofisicaX-rayscompact object0103 physical sciencesElectronicOptical and Magnetic MaterialsElectrical and Electronic EngineeringSpectral resolutionInstrumentation and Methods for Astrophysics (astro-ph.IM)dense hadronic matterSensors010308 nuclear & particles physicsX-ray imagingAstronomyAccretion (astrophysics)[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Neutron star13. Climate actionx-ray and γ-ray instrumentation; neutron stars; dense hadronic matter[ PHYS.ASTR.IM ] Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Gamma-ray burstastro-ph.IM
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Bezpieczeństwo socjalne jako element polityki społecznej samorządu terytorialnego w Niemczech

2018

Samorząd terytorialny w Niemczech jest jedną z najważniejszych części administracji publicznej w Niemczech, jest praktycznie jego podstawą. Posiada szeroko zakreśloną gwarancję konstytucyjną i równie rozległą autonomię. Prawo do samorządności mają nie tylko gminy, powiaty, związki gmin i okręgi w Bawarii, które posiadają pełną demokratyczną legitymizację opartą na głosowaniu obywateli, ale również i takich podmiotach, które nie mają tego typu demokratycznego umocowania. Do nich zalicza się specjalne formy samorządności terytorialnej - związki komunalne wyższego rzędu. Jednym z zadań realizowanych przez samorząd terytorialny w Niemczech jest polityka społeczna. Władze samorządowe, opierając …

związek celowyyouthpowiatspecial-purpose associationdziecibezpieczeństwo socjalnesick personsniepełnosprawniNiemcyhigher-profile municipal unionosoby starszesocial policydistrict (county)młodzieżpolityka społecznachildrenelderly personszwiązek komunalny wyższego rzęduGermanyosoby chorelocal governmentsamorząd terytorialnysocial securitydisabled personsChorzowskie Studia Polityczne
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