Search results for "Estela"

showing 8 items of 8 documents

Roman inscriptions from Paterna, Valencia, and Riba-Roja de Túria (Territorium of Valentia, Hispania Citerior)

2014

Presentamos en estas páginas once nuevas inscripciones romanas sobre diversos soportes, que han aparecido en la última década en diferentes excavaciones en localidades próximas a Valencia y en la propia ciudad, todas ellas dentro del territorium de la antigua Valentia. This article presents eleven new Roman inscriptions on various supports that were found in the last decade in different excavations in locations situated in the vicinity of Valencia and in the city itself, all of them within the territorium of the ancient city of Valentia.

ArcheologyRoman inscriptionsFunerary monumentsarqueologíaarchaeologyArqueologiaBroncelcsh:Auxiliary sciences of historyBronzeInstrumentum domesticumlcsh:Clcsh:Archaeologylcsh:CC1-960Historia AntiguaEstelaPonderalesInscripciones romanasPoundsSagvntum
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Photometric and spectroscopic variability of the B5IIIe star HD 171219

2017

We analyzed the star HD 171219, one of the relatively bright Be stars observed in the seismo field of the CoRoT satellite, in order to determine its physical and pulsation characteristics. Classical Be stars are main-sequence objects of mainly B-type, whose spectra show, or have shown at some epoch, Balmer lines in emission and an infrared excess. Both characteristics are attributed to an equatorially concentrated circumstellar disk fed by non-periodic mass-loss episodes (outbursts). Be stars often show nonradial pulsation gravity modes and, as more recently discovered, stochastically excited oscillations. Applying the CLEANEST algorithm to the high-cadence and highly photometrically precis…

Stars: individual: HD 171219Stars: emission-line BeAstrophysics::High Energy Astrophysical PhenomenaFísica matemàticaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesSpectral lineStars: early-typesymbols.namesakeearly-type [Stars]Stars: oscillationsStars: rotation0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsVariation (astronomy)010303 astronomy & astrophysicsSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsComputingMilieux_MISCELLANEOUSLine (formation)Physics[PHYS]Physics [physics]Infrared excess010308 nuclear & particles physicsASTROFÍSICA ESTELARBalmer seriesFísicaAstronomy and AstrophysicsoscillationsStars: rotation [Stars]Light curveCiència EnsenyamentStarsAstrophysics - Solar and Stellar Astrophysicsindividual: HD 171219 [Stars]emission-line Be [Stars]13. Climate actionSpace and Planetary ScienceExcited statesymbolsAstrophysics::Earth and Planetary Astrophysics[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
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Breve comentario sobre la lectura "Pinax" en la Estela ática número VII

1996

UNESCO::HISTORIA::Historia por épocas::Historia antiguaBreve comentario sobre la lectura "Pinax" en la Estela ática número VII ArtículoHumanidadesen la Estela ática número VII ArtículoGrupo CBreve comentario sobre la lectura &quotPinax&quot:HISTORIA::Historia por épocas::Historia antigua [UNESCO]Historia
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SDSS-III: Massive Spectroscopic Surveys of the Distant Universe, the Milky Way Galaxy, and Extra-Solar Planetary Systems

2011

Building on the legacy of the Sloan Digital Sky Survey (SDSS-I and II), SDSS-III is a program of four spectroscopic surveys on three scientific themes: dark energy and cosmological parameters, the history and structure of the Milky Way, and the population of giant planets around other stars. In keeping with SDSS tradition, SDSS-III will provide regular public releases of all its data, beginning with SDSS DR8 (which occurred in Jan 2011). This paper presents an overview of the four SDSS-III surveys. BOSS will measure redshifts of 1.5 million massive galaxies and Lya forest spectra of 150,000 quasars, using the BAO feature of large scale structure to obtain percent-level determinations of the…

Astrofísicaplanets and satellites: detection[PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]Milky WayFOS: Physical sciencesEspectros astronômicosAstrophysics::Cosmology and Extragalactic AstrophysicsSurveys01 natural sciencesevolution [Galaxy]Movimento estelarsurveysPlanetBulge0103 physical sciencesPhysical Sciences and MathematicsAstrophysics::Solar and Stellar AstrophysicsMatéria escuraobservations [Cosmology]Instrumentation and Methods for Astrophysics (astro-ph.IM)Tecnicas astronomicas010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsMapeamentos astronômicosAglomerados de galaxiasPlanetas extrasolaresPhysicsGalaxy: evolutionCosmologia010308 nuclear & particles physicsGiant planetAstrophysics::Instrumentation and Methods for AstrophysicsFísicaAstronomyAstronomy and AstrophysicsQuasarComposicao estelarPlanetary systemEspectros estelaresRedshiftGalaxy[SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM]detection [Planets and satellites]Space and Planetary Sciencecosmology: observationsAstrophysics::Earth and Planetary AstrophysicsAstrophysics - Instrumentation and Methods for Astrophysics
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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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Una estela ibèrica trobada a Atzeneta del Maestrat (l'Alt Maestrat, Castelló)

2017

We present the finding of an Iberian stele in the village of Atzeneta del Maestrat (Castellón). It is decorated with a cuirass disc on its front face, motif that is represented for the first time in the Iberian steles of the Valencian Country. Due to its characteristics, we connect this monument with the group of steles of Bajo Aragón, where we find the same motives in villages such as Vallderoures and Cretas (Teruel).

Cultura ibérica; monumento funerario; estela; disco-corazafunerary monumentestelaIberian culture; funerary monument; stele; disc cuirassCultura ibéricaIberian cultureArqueologiadisco-corazastelemonumento funerariodisc cuirassQuaderns de prehistòria i arqueologia de Castelló
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La estela de Juan de Juanes en el sureste español: el pintor Jerónimo de Córdoba (1537-1601)

2014

UNESCO::CIENCIAS DE LAS ARTES Y LAS LETRAS:CIENCIAS DE LAS ARTES Y LAS LETRAS [UNESCO]el pintor Jerónimo de Córdoba (1537-1601) Hernández Guardiola [0211-5808 9678 Archivo de arte valenciano 385455 2014 95 4935219 La estela de Juan de Juanes en el sureste español]0211-5808 9678 Archivo de arte valenciano 385455 2014 95 4935219 La estela de Juan de Juanes en el sureste español: el pintor Jerónimo de Córdoba (1537-1601) Hernández GuardiolaLorenzo 63 79
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Invocaciones duplicadas a los dioses Manes en inscripciones romanas de Hispania

2018

Presentamos en estas páginas ocho testimonios de inscripciones romanas que muestran la repetición de la fórmula D(is) M(anibus) s(acrum) o D(is) M(anibus). Todos los textos pueden ser datados entre los ss. II y III. La distribución geográfica de estos textos demuestra que se trata de testimonios aislados y que no guardan entre ellos ninguna relación. This article presents eight Roman inscriptions found in Hispania with reiteration of epigraphic formula D(is) M(anibus) s(acrum) or D(is) M(anibus). All these testimonies can be dated between the II and III centuries A.D. The geographical distribution shows isolated samples without connection. Este trabajo se ha realizado en el marco del proyec…

ArcheologyUNESCO::HISTORIAHispania CiteriorRoman epigraphyFunerary monumentsEpigraphic formulaBaeticaEpigrafía romanaMonumentos funerariosEstelas:HISTORIA [UNESCO]Historia AntiguaFormularios epigráficosStelaeSAGVNTVM. Papeles del Laboratorio de Arqueología de Valencia
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