Search results for "raga"

showing 10 items of 1852 documents

Nel segno di Zeus: su alcuni louteria fittili da Akragas

2018

The study considers some louteria from Agrigento (from the Sanctuary of Zeus Olympios and the so-called Sanctuary of chthonic deities), dated from the sixth to the fifth century BC. In particular we propose a reading of the images that decorate these basins in relation to the sacred contexts in which they were used, paying particular attention to a series of louteria with running quadrigae and winged figures and an example depicting the transport of Achilles’ weapons by the Nereids. Thus symbolic imagerie which refers to the rituals and cults practised in these sacred spaces is reconstructed.

Akragas louterion NereidsSettore L-ANT/07 - Archeologia Classica
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Il santuario di Zeus Olympios nel quadro urbano dell’antica Akragas

2019

The sanctuary of Zeus Olympios at Agrigento has been not perceived in its entirety till now. As a matter of fact, while the temple attracted the scholars’ interest, due to its outstanding features, the buildings surrounding it were referred to residential (W), military (S) and civic (“agora” E/NE) functions. Besides, a sacellum and a pool on the south-eastern side were attributed to the age of Timoleon, later than the main architectural phase. However, the new stratigraphical data allow us to refer all the structures in the southern area to a coherent building program carried out from 480 to 450 BC Starting from this evidence, the paper aims at redefining the whole context, putting it in ur…

Akragas sanctuary Zeus Olympios urban planningSettore L-ANT/07 - Archeologia Classica
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Considerazioni sull’approvvigionamento e smaltimento idrico dell’area centro-occidentale della Collina dei Templi di Agrigento in età classica

2020

A partire dalle recenti indagini dell’Università di Palermo nell’area tra i Templi di Zeus e di Eracle ad Agrigento, e dalla revisione condotta da Giovanni Luca Furcas dei sistemi idrici akragantini, si propongono alcune considerazioni su un importante aspetto della vita dei complessi sacri, ancora non adeguatamente approfondito. In particolare si cercherà di cogliere il legame tra l’infrastrutturazione idrica e lo sviluppo diacronico dei santuari nella porzione sud-occidentale della città. The paper examines the water supply and disposal in the central-western part of the Collina dei Templi at Agrigento. Starting from the current investigations by the team of the University of Palermo in t…

Akragas sistemi idraulici santuariAkragas hydraulic systems sanctuariesSettore L-ANT/07 - Archeologia Classica
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Off-line coupling of multidimensional immunoaffinity chromatography and ion mobility spectrometry: A promising partnership.

2015

The extreme specificity of immunoaffinity chromatography (IAC) columns coupled to the high sensitivity of ion mobility spectrometry (IMS) measurements makes this combination really useful for rapid, selective, and sensitive determination of a high variety of analytes in different samples. The capabilities of the IAC-IMS coupling have been highlighted under three different scenarios: (i) multiclass residue analysis using a single IAC column, (ii) multiclass residue analysis using stacked IAC columns, and (iii) isomer analysis. In the first case, the determination of three strobilurin fungicides - azoxystrobin, picoxystrobin, and pyraclostrobin - in water and strawberry juice was considered, …

AnalyteIon-mobility spectrometryPyridinesAnalytical chemistryWineBiochemistryFragariaSensitivity and SpecificityChromatography AffinityAnalytical Chemistrychemistry.chemical_compoundWineResidue (complex analysis)ChromatographyElutionOrganic ChemistryWaterStereoisomerismGeneral MedicineStrobilurinsFungicides IndustrialFruit and Vegetable JuicesPyrimidineschemistryAcrylatesAzoxystrobinStrobilurinMethacrylatesPyrazolesPyrimethanilCarbamatesJournal of chromatography. A
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Optical and ultraviolet pulsed emission from an accreting millisecond pulsar

2021

Ambrosino, F., et al.

Angular momentum010504 meteorology & atmospheric sciencesAstrophysics::High Energy Astrophysical PhenomenaMagnetosphereFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesLuminosityNeutron starsSettore FIS/05 - Astronomia E AstrofisicaPulsarMillisecond pulsar0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena0105 earth and related environmental sciencesPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)Astronomy and AstrophysicsAccretion (astrophysics)Particle accelerationNeutron starAstrophysics::Earth and Planetary AstrophysicsAstrophysics - High Energy Astrophysical Phenomena
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Mass Accretion Processes in Young Stellar Objects: Role of Intense Flaring Activity

2014

According to the magnetospheric accretion scenario, young low-mass stars are surrounded by circumstellar disks which they interact with through accretion of mass. The accretion builds up the star to its final mass and is also believed to power the mass outflows, which may in turn have a significant role in removing the excess angular momentum from the star-disk system. Although the process of mass accretion is a critical aspect of star formation, some of its mechanisms are still to be fully understood. On the other hand, strong flaring activity is a common feature of young stellar objects (YSOs). In the Sun, such events give rise to perturbations of the interplanetary medium. Similar but mo…

Angular momentumMHDStars: flareAstrophysics::High Energy Astrophysical PhenomenaYoung stellar objectFOS: Physical sciencesInterplanetary mediumAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsAcoustics and UltrasonicAccretion accretion diskIntermediate polarAstrophysics::Solar and Stellar AstrophysicsX-rays: starSolar and Stellar Astrophysics (astro-ph.SR)Astrophysics::Galaxy AstrophysicsNuclear and High Energy PhysicGeneral Environmental SciencePhysicsRadiationStar formationAstronomyAccretion (astrophysics)StarsAstrophysics - Solar and Stellar Astrophysicslcsh:TA1-2040Space and Planetary ScienceStars: circumstellar matterGeneral Earth and Planetary SciencesCircumstellar dustAstrophysics::Earth and Planetary Astrophysicslcsh:Engineering (General). Civil engineering (General)Stars: pre-main-sequenceActa Polytechnica CTU Proceedings
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Linear and cyclic radio k-labelings of trees

2007

International audience; Motivated by problems in radio channel assignments, we consider radio k-labelings of graphs. For a connected graph G and an integer k ≥ 1, a linear radio k-labeling of G is an assignment f of nonnegative integers to the vertices of G such that |f(x)−f(y)| ≥ k+1−dG(x,y), for any two distinct vertices x and y, where dG(x,y) is the distance between x and y in G. A cyclic k-labeling of G is defined analogously by using the cyclic metric on the labels. In both cases, we are interested in minimizing the span of the labeling. The linear (cyclic, respectively) radio k-labeling number of G is the minimum span of a linear (cyclic, respectively) radio k-labeling of G. In this p…

Applied Mathematics010102 general mathematicsGraph theory[ INFO.INFO-DM ] Computer Science [cs]/Discrete Mathematics [cs.DM]Astrophysics::Cosmology and Extragalactic Astrophysics0102 computer and information sciences[INFO.INFO-DM]Computer Science [cs]/Discrete Mathematics [cs.DM]Span (engineering)01 natural sciencesUpper and lower boundsCombinatoricsGraph theory[INFO.INFO-DM] Computer Science [cs]/Discrete Mathematics [cs.DM]IntegerRadio channel assignment010201 computation theory & mathematicsCyclic and linear radio k-labelingMetric (mathematics)Path (graph theory)Discrete Mathematics and CombinatoricsOrder (group theory)0101 mathematicsMSC 05C15 05C78ConnectivityMathematics
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Absolute kinematics of radio-source components in the complete S5 polar cap sample: IV. Proper motions of the radio cores over a decade and spectral …

2016

We have carried out a high-precision astrometric analysis of two very-long-baseline-interferometry (VLBI) epochs of observation of the 13 extragalactic radio sources in the complete S5 polar cap sample. The VLBI epochs span a time baseline of ten years and enable us to achieve precisions in the proper motions of the source cores up to a few micro-arcseconds per year. The observations were performed at 14.4 GHz and 43.1 GHz, and enable us to estimate the frequency core-shifts in a subset of sources, for which the spectral-index distributions can be computed. We study the source-position stability by analysing the changes in the relative positions of fiducial source points (the jet cores) ove…

AstrofísicaActive galactic nucleusAstrometriaAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsKinematics01 natural sciencesStability (probability)Radio continuum: generalBinary black hole0103 physical sciencesVery-long-baseline interferometry010306 general physicsInstrumentation and Methods for Astrophysics (astro-ph.IM)010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsJet (fluid)general [Radio continuum]general [BL Lacertae objects]Astrophysics::Instrumentation and Methods for AstrophysicsAstronomy and Astrophysicsgeneral [Quasars]BL Lacertae objects: generalAstrometryAstrometryAstrophysics - Astrophysics of GalaxiesQuasars: generalGravitational lensSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Techniques: interferometricinterferometric [Techniques]Astrophysics - Instrumentation and Methods for Astrophysics
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The gamma-ray emitting radio-loud narrow-line Seyfert 1 galaxy PKS 2004-447 I. The X-ray View

2015

As part of the TANAMI multiwavelength progam, we discuss new X-ray observations of the $\gamma$-ray and radio-loud Narrow Line Seyfert galaxy ($\gamma$-NLS1) PKS 2004-447. The active galaxy is a member of a small sample of radio-loud NLS1s detected in $\gamma$-rays by the Fermi Large Area Telescope. It is the radio-loudest and only southern-hemisphere source in this sample. We present results from our X-ray monitoring program comprised of Swift snapshot observations from 2012 through 2014 and two new X-ray observations with XMM-Newton in 2012. We analyze the X-ray spectrum and variability of this peculiar source using supplementary archival data from 2004 and 2011. The (0.5-10) keV spectrum…

AstrofísicaActive galactic nucleusAstronomyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio spectrumlaw.inventionTelescopeRelativistic beaminglaw0103 physical sciencesVery-long-baseline interferometryBlazar010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)010308 nuclear & particles physicsAstronomy and AstrophysicsMonitoring programAstrophysics - Astrophysics of GalaxiesGalaxySpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)AstronomiaComputingMethodologies_DOCUMENTANDTEXTPROCESSINGAstrophysics - High Energy Astrophysical Phenomena
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LeMMINGs III. The e-MERLIN legacy survey of the Palomar sample: exploring the origin of nuclear radio emission in active and inactive galaxies throug…

2021

Full list of authors: Baldi, R. D.; Williams, D. R. A.; Beswick, R. J.; McHardy, I.; Dullo, B. T.; Knapen, J. H.; Zanisi, L.; Argo, M. K.; Aalto, S.; Alberdi, A.; Baan, W. A.; Bendo, G. J.; Fenech, D. M.; Green, D. A.; Klöckner, H. -R.; Körding, E.; Maccarone, T. J.; Marcaide, J. M.; Mutie, I.; Panessa, F.; Pérez-Torres, M. A.; Romero-Cañizales, C.; Saikia, D. J.; Saikia, P.; Shankar, F.; Spencer, R. E.; Stevens, I. R.; Uttley, P.; Brinks, E.; Corbel, S.; Martí-Vidal, I.; Mundell, C. G.; Pahari, M.; Ward, M. J.

AstrofísicaActive galactic nucleusAstronomyAstrophysics::High Energy Astrophysical Phenomenanuclei [galaxies]jets [galaxies]Doubly ionized oxygenFOS: Physical sciencesAstrophysicsF500Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio continuum: galaxiesLuminosityAstrophysical jetSubatomic Physics0103 physical sciencesAstronomy Astrophysics and CosmologyAstrophysics::Solar and Stellar AstrophysicsConnection (algebraic framework)010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsGalaxies: nucleiAstronomia ObservacionsHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]Galaxies: star formation010308 nuclear & particles physicsAstronomy and AstrophysicsGalaxies: activeAstrophysics - Astrophysics of Galaxiesgalaxies [radio continuum]Accretion (astrophysics)Galaxy[SDU]Sciences of the Universe [physics]Meteorology and Atmospheric SciencesSpace and Planetary ScienceGalaxies: jetsAstrophysics of Galaxies (astro-ph.GA)active [galaxies]Production (computer science)star formation [galaxies]Astrophysics - High Energy Astrophysical Phenomena
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