Search results for "GAL"

showing 10 items of 9260 documents

Studying the Cognitive Map of the US States: Ideology and Prosperity Stereotypes Predict Interstate Prejudice

2018

What are the spontaneous stereotypes that U.S. citizens hold about the U.S. states? We complemented insights from theory-driven approaches to this question with insights from a novel data-driven approach. Based on pile sorting and spatial arrangement similarity ratings for the states, we computed two cognitive maps of the states. Based on ratings for the states on ∼20 candidate dimensions, we interpreted the dimensions that spanned the two maps (Studies 1 and 2). Consistent with the agency/socioeconomic success, conservative-progressive beliefs, and communion (ABC) model of spontaneous stereotypes, these dimensions that participants spontaneously used to rate the states’ similarity included…

spontaneous stereotypesCognitive mapSocial Psychologymedia_common.quotation_subject05 social sciencesAgency (philosophy)ideologyClinical psychology050109 social psychologyprosperity050105 experimental psychologyAbc modelABC modelSimilarity (psychology)U.S. states0501 psychology and cognitive sciencesProsperityIdeologyPsychologySocial psychologySocioeconomic statusPrejudice (legal term)media_common
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Dwa poselstwa oboźnego litewskiego Ignacego Ogińskiego na dwór petersburski. Rola Litwinów w kontaktach dyplomatycznych z Rosją w latach 1711-1763

2020

W artykule przedstawiona została problematyka funkcjonowania dyplomacji Rzeczypospolitej w stosunkach z Rosją w latach 1711-1763. Za dolną cezurę przyjęto poselstwo Marcjana Dominika Wołłowicza do cara Piotra I, które jednoznacznie zakończyło okres separatystycznych litewskich działań dyplomatycznych z pierwszej dekady XVIII wieku. Przywrócona została zasada prowadzenia wspólnej polityki zagranicznej Korony i Wielkiego Księstwa z uwzględnieniem większego zainteresowania Litwinów stosunkami z Rosją. Znajdowało to swój wyraz w przygotowywaniu instrukcji i innych dokumentów poselskich przez kancelarie litewskie, jak też w zwyczajowym udziale w każdej misji Litwina jako eksponowanego członka po…

spory pograniczneskutki wojny rosyjsko-osmańskiej 1736-1739Cerkiew prawosławnaImperium RosyjskieWielkie Księstwo LitewskieKościół katolickiIgnacy OgińskiDyplomacja Rzeczypospolitej Obojga NarodówKsięstwo Kurlandii i Semigalii
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Galvinieka atbildības problemātiskie aspekti.

2018

Bakalaura darba tēmas nosaukums ir „Galvinieka atbildības problemātiskie aspekti”. Galvojums ir viens no saistību pastiprināšanas veidiem. Lai attīstītu ekonomisko aktivitāti, jau senajā Romā, galvojums kalpoja, kā personisks garants saistību izpildīšanai. To nodrošināja trešā persona, kura ar savu galvu galvoja kreditoram par citas personas parādu. Zinātniskā darba mērķis ir izpētīt galvinieka tiesības un pienākumus fiziskas maksātnespējas procesos, normatīvo regulējumu, saistību dzēšanu, pastāvošo tiesu praksi un tiesībzinātnieku viedokļus, izzināt iespējamos strīdīgos jautājumus pastāvošajās normās un tiesu spriedumos. Lai sasniegtu darba mērķi ir noteikti sekojoši uzdevumi: 1)izpētīt ga…

spēkā esoša saistībatiesneša tiesībasdarījuma pušu paustā gribatiesību tālākveidošanaekspromisoriskais galvinieksJuridiskā zinātne
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Ilustratīvie elementi spēļu kāršu dizainā

2021

Diplomdarba tēma ir “Ilustratīvie elementi spēļu kāršu dizainā”. Balstoties uz teorētiskajā daļā uzzināto un empīriskajā daļā izpētīto, darba mērķis ir izveidot jaunu spēļu kāršu dizainu galda spēlei “Saboteur” izmantojot ilustratīvos elementus, kas ir raksturīgi tradicionālajām spēļu kārtīm. Teorētiskajā daļā ir aprakstīta tradicionālo spēļu kāršu vēsture, kā arī ilustratīvie elementi, kas ir atrodami spēļu kāršu dizainā, to paskaidrojums un nozīme. Tiek izvirzīti vizuālā dizaina principi uz kuriem balstoties būtu iespējams izveidot funkcionālu spēļu kāršu dizainu. Empīriskajā daļā tika veikta 10 dažādu galda spēļu kāršu komplektu vizuālā dizaina analīze, lai izprastu teorētiskajā daļā min…

spēļu kārtisgalda spēlesMākslas zinātnegrafiskais dizainsvizuālā stilistikailustratīvie elementi
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The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST)

2007

(abridged:) The XMM-Newton Extended Survey of the Taurus Molecular Cloud (XEST) surveys the most populated ~5 square degrees of the Taurus star formation region, using the XMM-Newton X-ray observatory to study the thermal structure, variability, and long-term evolution of hot plasma, to investigate the magnetic dynamo, and to search for new potential members of the association. Many targets are also studied in the optical, and high-resolution X-ray grating spectroscopy has been obtained for selected bright sources. The X-ray spectra have been coherently analyzed with two different thermal models (2-component thermal model, and a continuous emission measure distribution model). We present ov…

stars : pre-main sequence010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaBrown dwarfFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesLuminosity[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Observatory0103 physical sciencesProtostarAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsstars : formationStar formationMolecular cloudAstrophysics (astro-ph)Astronomy and AstrophysicsAccretion (astrophysics)Starsgravitational waves13. Climate actionSpace and Planetary ScienceX-rays : star
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Stochastic gravito-inertial modes discovered by CoRoT in the hot Be star HD 51452

2012

International audience; Context. Be stars are rapidly rotating stars with a circumstellar decretion disk. They usually undergo pressure and/or gravity pulsation modes excited by the κ-mechanism, i.e. an effect of the opacity of iron-peak elements in the envelope of the star. In the Milky Way, p-modes are observed in stars that are hotter than or equal to the B3 spectral type, while g-modes are observed at the B2 spectral type and cooler. Aims. We observed a B0IVe star, HD 51452, with the high-precision, high-cadence photometric CoRoT satellite and high-resolution, ground-based HARPS and SOPHIE spectrographs to study its pulsations in great detail. We also used the lower resolution spectra a…

starsBe -stars010504 meteorology & atmospheric sciencesBe starK-type main-sequence staroscillations -starsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsrotation01 natural sciences0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsStellar structureindividual010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysics0105 earth and related environmental sciences[PHYS]Physics [physics]PhysicsASTROFÍSICA ESTELARStellar rotationFlare starAstronomyAstronomy and AstrophysicsLight curveESPECTROSCOPIAHD 51452 -starsStarsT Tauri star13. Climate actionSpace and Planetary ScienceAstrophysics::Earth and Planetary Astrophysicsemission-line[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Astronomy & Astrophysics
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High Energy Emission and its Variability in Young Stellar Objects

2019

Young stars show a variety of highly energetic phenomena, from accretion and outflow processes to hot coronal plasmas confined in their outer atmosphere, all regulated by the intense stellar magnetic fields. Many aspects on each of these phenomena are debated, but, most notably, their complex mutual interaction remains obscure. In this work I report how these phenomena are simultaneously responsible for the high-energy emission from young stars, with a special focus on the expected and observed variability in the X-ray band. Investigating variations in the X-ray emission from young stars allows us to pose constraints on flare and coronal plasma properties, coronal heating, accretion stream …

starsYoung stellar objectAstrophysics::High Energy Astrophysical PhenomenaMagnetosphereFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural scienceslaw.inventionX-raySettore FIS/05 - Astronomia E Astrofisicaaccretionstarlaw0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicspremain sequenceSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsactivityAstronomy and AstrophysicsPlasmaAccretion (astrophysics)StarsT Tauri starAstrophysics - Solar and Stellar AstrophysicsSpace and Planetary ScienceT Tauri starOutflowAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical PhenomenaFlare
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Chemical Cartography with APOGEE: Multi-element Abundance Ratios

2019

We map the trends of elemental abundance ratios across the Galactic disk, spanning R = 3-15 kpc and midplane distance |Z|= 0-2 kpc, for 15 elements in a sample of 20,485 stars measured by the SDSS/APOGEE survey (O, Na, Mg, Al, Si, P, S, K, Ca, V, Cr, Mn, Fe, Co, Ni). Adopting Mg rather than Fe as our reference element, and separating stars into two populations based on [Fe/Mg], we find that the median trends of [X/Mg] vs. [Mg/H] in each population are nearly independent of location in the Galaxy. The full multi-element cartography can be summarized by combining these nearly universal median sequences with our measured metallicity distribution functions and the relative proportions of the lo…

stars: abundances010504 meteorology & atmospheric sciencesMilky WayMetallicityPopulationFOS: Physical sciences01 natural sciencesGalaxy: diskStellar nucleosynthesisNucleosynthesis0103 physical scienceseducation010303 astronomy & astrophysicsnuclear reactions0105 earth and related environmental sciencesPhysicseducation.field_of_studyabundancesnucleosynthesisAstronomy and AstrophysicsAstrophysics - Astrophysics of GalaxiesGalaxySupernova13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Galaxy: abundancesSupernova nucleosynthesis[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]CartographyThe Astrophysical Journal
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The Gaia-ESO Survey: impact of extra mixing on C and N abundances of giant stars

2018

The GES survey using FLAMES at the VLT has obtained high-resolution UVES spectra for a large number of giant stars, allowing a determination of the abundances of the key chemical elements C and N at their surface. The surface abundances of these chemical species are well-known to change in stars during their evolution on the red giant branch after the first dredge-up episod, as a result of extra-mixing phenomena. We investigate the effects of thermohaline mixing on C and N abundances using the first comparison between the GES [C/N] determinations with simulations of the observed fields using a model of stellar population synthesis. We explore the effects of thermohaline mixing on the chemic…

stars: abundances010504 meteorology & atmospheric sciencesStellar populationMetallicityFOS: Physical sciencesabundances ; stars: evolution ; galaxy: stellar content ; galaxy: abundances ; astrophysics - solar and stellar astrophysics [stars]AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAstronomi astrofysik och kosmologi0103 physical sciencesAstrophysics::Solar and Stellar Astrophysicsstellar content [Galaxy]Astronomy Astrophysics and Cosmologystars: evolution14. Life underwater010303 astronomy & astrophysicsStellar evolutionSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy Astrophysics0105 earth and related environmental sciencesPhysicsGalaxy: stellar contentabundances [Galaxy]Astronomy and AstrophysicsGiant starRed-giant branchabundances [stars]StarsAstrophysics - Solar and Stellar Astrophysics13. Climate actionSpace and Planetary ScienceGlobular clusterevolution [stars]Galaxy: abundancesAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Open cluster
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Simbol-X capability of detecting the non-thermal emission of stellar flares.

2008

We investigate the capability of detecting, with Simbol-X, non-thermal emission during stellar flares, and distinguishing it from hot thermal emission. We find that flare non-thermal emission is detectable when at least ~20 cts are detected with the CZT detector in the 20-80 keV band. Therefore Simbol-X will detect the non-thermal emission from some of the X-ray brightest nearby stars, whether the thermal vs. non-thermal relation, derived for solar flares, holds.

stars: coronaeSettore FIS/05 - Astronomia E AstrofisicaAstrophysics::High Energy Astrophysical PhenomenaAstrophysics (astro-ph)stars: activityFOS: Physical sciencesAstrophysics::Solar and Stellar AstrophysicsAstrophysics::Earth and Planetary AstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAstrophysics::Galaxy Astrophysics
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