Search results for "STELLA"

showing 10 items of 1995 documents

«La discordia en los casados» de Lope de Vega y su modelo italiano.

1998

El estudio analítico que Romera Pintor presenta en este artículo desarrolla una metodología crítica comparada, debidamente documentada, que ofrece unas conclusiones innovadoras en el marco de la investigación en torno a Giraldi. Romera Pintor demuestra, mediante el pormenorizado análisis comparativo entre la 'Selene' de Giraldi y la obra de Lope, que Giraldi fue fuente de inspiración para la obra de Lope.

lcsh:Philology. Linguisticslcsh:French literature - Italian literature - Spanish literature - Portuguese literaturelcsh:P1-1091lcsh:PQ1-3999Literatura castellana 1500-1700 Segle d'Or
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Los libros de viajes medievales castellanos : Introducción al panorama crítico actual: ¿cuántos libros de viajes medievales castellanos?

1991

Se examinan y estudian algunos de los principales libros de viajes de la literatura castellana medieval, en su contexto europeo, con especial atención al 'Libro del conosçimiento', la 'Embajada a Tamorlán' y el 'Tratado' de Pero Tafur. Se analiza los textos, en su contenido y en su poética de pertenencia a un género híbrido, que combina lo narrativo y descriptivo con lo novelesco, y la voz autobiográfica con la necesidad de objetivación didáctica.

lcsh:Philology. Linguisticslcsh:P1-1091lcsh:PC1-5498lcsh:Romanic languagesLiteratura castellana
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La clase de lengua en secundaria como aula de E/LE: cómo aplicar algunas herramientas de L2

2013

El alumnado no nativo en secundaria obligatoria (ESO) requiere una atención y una adaptación curricular específicas, por lo que el profesorado ha de emplear las estrategias necesarias para que pueda adquirir en poco tiempo la lengua vehicular, imprescindible para poder progresar en el resto de materias. La obligatoriedad de este nivel educativo y las exigencias para poder promocionar dificultan el proceso, especialmente a la hora de aplicar los criterios de evaluación y de calificar al alumno. Una alternativa complementaria a la evaluación oficial la constituyen los materiales y herramientas de E/LE, puesto que permiten valorar los progresos lingüísticos del alumno y comprobar el grado de c…

lcsh:Philology. Linguisticslcsh:P1-1091lengua castellana:PEDAGOGÍA [UNESCO]adaptaciones curricularesL1 y L2lcsh:LUNESCO::PEDAGOGÍAE/LElcsh:Education
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Los libros de caballerías como obras didácticas según dos prólogos artúricos: Baladro del sabio Merlín y Tristán de Leonís

2013

El prólogo es uno de los paratextos que se consolidó en la narrativa caballeresca con la llegada de la imprenta. El baladro del sabio Merlín (1498) y el Tristán de Leonís (1501), impresos por Juan de Burgos, son ejemplos tempranos de la importancia del prólogo. Ambas obras proceden de una larga tradición manuscrita derivada de textos franceses. Las versiones impresas castellanas reelaboran dicha tradición. En ambas obras, se agregó un prólogo. En dicha sección, por medio de diferentes recursos, se resalta el valor didáctico, además del entretenimiento, que los libros de caballerías ofrecían a sus lectores. Este trabajo estudia cómo, por medio de estos prólogos, se buscó orientar la lectura …

libros de caballerías castellanosprólogos; función didáctica; libros de caballerías castellanos; Juan de Burgosanálisis de textosfilología; filología española; literatura; literatura medieval; literatura románica; análisis de textosliteratura medievalliteratura románicafilología españolaliteraturaprólogosfunción didácticafilologíaJuan de Burgos
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Spatially Resolved Broadband Synchrotron Emission from the Nonthermal Limbs of SN1006

2018

We present ~400ks NuSTAR observations of the northeast (NE) and southwest (SW) non-thermal limbs of the Galactic SNR SN1006. We discovered three sources with X-ray emission detected at >50keV. Two of them are identified as background AGN. We extract the NuSTAR spectra from a few regions along the non-thermal limbs and jointly analyze them with the XMM-Newton spectra and the radio data. The broad-band radio/X-ray spectra can be well described with a synchrotron emission model from a single population of CR electrons with a power law energy distribution and an exponential cutoff. The power law index of the electron particle distribution function (PDF) is ~1.88-1.95 for both the NE and SW l…

media_common.quotation_subjectAstrophysics::High Energy Astrophysical PhenomenaPopulationFOS: Physical sciencesAstrophysicsElectronAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesAsymmetryPower lawSpectral linecosmic rays0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrumeducation010303 astronomy & astrophysicsAstrophysics::Galaxy Astrophysicsmedia_commonISM: supernova remnantsacceleration of particlesHigh Energy Astrophysical Phenomena (astro-ph.HE)Physicseducation.field_of_study010308 nuclear & particles physicsAstronomy and Astrophysicsshock wavesAstronomy and Astrophysicradiation mechanisms: non-thermalX-rays: ISMMagnetic fieldSpace and Planetary ScienceAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Lepton
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Discovery of slow X-ray pulsations in the high-mass X-ray binary 4U 2206+54

2008

Context. The source 4U 2206+54 is one of the most enigmatic high-mass X-ray binaries. In spite of intensive searches, X-ray pul- sations have not been detected in the time range 10−3–103 s. A cyclotron line at ∼30 keV has been suggested by various authors but never detected with significance. The stellar wind of the optical companion is abnormally slow. The orbital period, initially reported to be 9.6 days, disappeared and a new periodicity of 19.25 days emerged. Aims. The main objective of our RXTE monitoring of 4U 2206+54 is to study the X-ray orbital variability of the spectral and timing parameters. The new long and uninterrupted RXTE observations allow us to search for long (∼1 h) puls…

media_common.quotation_subjectAstrophysics::High Energy Astrophysical Phenomenapulsars : general [Stars]X-ray binaryFOS: Physical sciencesOrbital eccentricityAstrophysicsAstrophysicsStars : early-type; Stars : emission-line Be; Stars : binaries : close; X-rays : binaries; Stars : pulsars : generalLuminosityearly-type [Stars]:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos X [UNESCO]UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Fuentes de Rayos XAstrophysics::Solar and Stellar AstrophysicsEccentricity (behavior)binaries : close [Stars]media_commonLine (formation)PhysicsAstrophysics (astro-ph)Astronomy and AstrophysicsOrbital periodLight curveNeutron starSpace and Planetary Scienceemission-line Be [Stars]binaries [X-rays]Astrophysics::Earth and Planetary AstrophysicsUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia::Estrellas [UNESCO]
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Lyman break and ultraviolet-selected galaxies at z ̃ 1-I. Stellar populations from the ALHAMBRA survey

2013

We take advantage of the exceptional photometric coverage provided by the combination of GALEX data in the ultraviolet (UV) and the ALHAMBRA survey in the optical and near-infrared to analyse the physical properties of a sample of 1225 GALEX-selected Lyman break galaxies (LBGs) at 0.8 ≲ z ≲ 1.2 that are located in the COSMOS field. This is the largest sample of LBGs studied in this redshift range to date. According to a spectral energy distribution (SED) fitting with synthetic stellar population templates, we find that LBGs at z ̃ 1 are mostly young galaxies with a median age of 341 Myr and have intermediate dust attenuation, (Es(B - V)) ̃ 0.20. Owing to the selection criterion, LBGs at z ̃…

media_common.quotation_subjectLibrary scienceAstrophysics::Cosmology and Extragalactic Astrophysicsstar formation [Galaxies]high-redshift [Galaxies]ExcellenceAstrophysics::Solar and Stellar Astrophysicsobservations [Cosmology]Astrophysics::Galaxy Astrophysicsmedia_commonPhysicsGalaxies: star formationphotometry [Galaxies]Cosmology: observationsGalaxies: high-redshiftAstronomyGalaxies: evolutionAstronomy and AstrophysicsGalaxies: photometryevolution [Galaxies]Galaxygalaxies [Ultraviolet]Space and Planetary ScienceUltraviolet: galaxiesAstrophysics::Earth and Planetary AstrophysicsAdministration (government)
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The VST Photometric Hα Survey of the Southern Galactic Plane and Bulge (VPHAS+)

2014

The VST Photometric Halpha Survey of the Southern Galactic Plane and Bulge (VPHAS+) is surveying the southern Milky Way in u, g, r, i and Halpha at 1 arcsec angular resolution. Its footprint spans the Galactic latitude range -5 < b < +5 at all longitudes south of the celestial equator. Extensions around the Galactic Centre to Galactic latitudes +/-10 bring in much of the Galactic Bulge. This ESO public survey, begun on 28th December 2011, reaches down to 20th magnitude (10-sigma) and will provide single-epoch digital optical photometry for around 300 million stars. The observing strategy and data pipelining is described, and an appraisal of the segmented narrowband Halpha filter in us…

media_common.quotation_subjectMilky WayAstronomyFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energyPhotometry (optics)BulgeQB460Astrophysics::Solar and Stellar AstrophysicsQCAstrophysics::Galaxy Astrophysicsmedia_commonQBPhysicsCelestial equatorWhite dwarfAstronomyAstronomy and AstrophysicsGalactic planeAstrophysics - Astrophysics of GalaxiesStars13. Climate actionSpace and Planetary ScienceSkyAstrophysics of Galaxies (astro-ph.GA)ComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstrophysics::Earth and Planetary Astrophysics
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The ALHAMBRA survey: Bayesian photometric redshifts with 23 bands for 3 deg2

2014

A. Molino et al.

media_common.quotation_subjectPhotometric systemAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsSurveyslaw.inventionPhotometry (optics)Telescopelawdistances and redshifts [Galaxies]Astrophysics::Solar and Stellar Astrophysicsdata analysis [Methods]Astrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSPhotometric redshiftmedia_commonPhysics[PHYS]Physics [physics]photometry [Galaxies]photometric [Techniques]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomyAstronomy and AstrophysicsCataloguesevolution [Galaxies]GalaxyRedshift13. Climate actionSpace and Planetary ScienceSkyMagnitude (astronomy)Astrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Carcinogenic aspect of xenobiotic molecules belonging to the peroxisome proliferator family.

1999

It is known that a short-term exposure of rat, mice or incubation of hepatic cells with fibrate molecules leads to increase in peroxisome number and cell hyperplasia. Further, long-term incubation of cells (at least a year) show transformed characteristics with foci and nodules. To explain the hepatocarcinogenic effect of peroxisome proliferators in rodents we studied the effect of peroxisome proliferators on rat liver oncogenes expression. Earlier, we reported an increase in liver and kidney mRNA level of c-myc and N-myc. Since several metabolic genes are activated by PPAR (peroxisome proliferators activated receptor) through a PPRE (peroxisome proliferator response element), we suggest th…

medicine.drug_classCarcinogenicity TestsResponse elementGuinea PigsPeroxisome proliferator-activated receptorPeroxisome ProliferationRodentiaFibrateBiologyXenobioticsGeneticsmedicineTumor Cells CulturedAnimalsHumansReceptorchemistry.chemical_classificationGeneral MedicineOncogenesPeroxisomeMolecular biologyCell biologyRatsCell Transformation NeoplasticchemistryHepatic stellate cellCarcinogensPeroxisome ProliferatorsCiprofibrateCell Divisionmedicine.drugHepatomegalyInternational journal of molecular medicine
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