Search results for "active"

showing 10 items of 5361 documents

Jet-torus connection in radio galaxies

2017

High-resolution Very-Long-Baseline Interferometry observations of active galactic nuclei have revealed asymmetric structures in the jets of radio galaxies. These asymmetric structures may be due to internal asymmetries in the jet, could be induced by the different conditions in the surrounding ambient medium including the obscuring torus, or a combination of the two. In this paper we investigate the influence of the ambient medium (including the obscuring torus) on the observed properties of jets from radio galaxies. We performed special-relativistic hydrodynamic (RHD) simulations of over-pressured and pressure-matched jets using the special-relativistic hydrodynamics code \texttt{Ratpenat}…

Active galactic nucleusRadio galaxyAstrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesGeneral Relativity and Quantum Cosmology (gr-qc)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesElectromagnetic radiationGeneral Relativity and Quantum Cosmology0103 physical sciencesVery-long-baseline interferometryRadiative transfer010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)Spectral index010308 nuclear & particles physicsAstronomy and AstrophysicsTorusAstrophysics - Astrophysics of Galaxies13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics - High Energy Astrophysical PhenomenaAstronomy & Astrophysics
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A new sample of large angular size radio galaxies

2004

We present in this paper a detailed study of a new sample of large angular size FR I and FR II radio galaxies and compare the properties of the two classes. As expected, a pure morphology based distinction of FR Is and FR IIs corresponds to a break in total radio power. The radio cores in FR Is are also weaker than in FR IIs, although there is not a well defined break power. We find that asymmetry in the structure of the sample members must be the consequence of anisotropies in the medium where the lobes expand, with orientation playing a minor role. Moreover, literature data and our observations at kiloparsec scales suggest that the large differences between the structures of FR I and FR I…

Active galactic nucleusRadio galaxyAstrophysics::High Energy Astrophysical Phenomenamedia_common.quotation_subjectPopulationFOS: Physical sciencesSample (statistics)Astrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsActive galaxies ; Nuclei Jets ; Radio continuumUNESCO::ASTRONOMÍA Y ASTROFÍSICAAstrophysicsAsymmetryNuclei JetsAngular diametereducationAstrophysics::Galaxy AstrophysicsLuminosity function (astronomy)media_commonPhysicseducation.field_of_studyAstrophysics (astro-ph)Astronomy and Astrophysics:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]GalaxyRadio continuumSpace and Planetary ScienceActive galaxiesUNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]Astronomy & Astrophysics
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Correlation of the highest-energy cosmic rays with nearby extragalactic objects.

2007

Using data collected at the Pierre Auger Observatory during the past 3.7 years, we demonstrated a correlation between the arrival directions of cosmic rays with energy above ~ 6x10^{19} electron volts and the positions of active galactic nuclei (AGN) lying within ~ 75 megaparsecs. We rejected the hypothesis of an isotropic distribution of these cosmic rays with at least a 99% confidence level from a prescribed a priori test. The correlation we observed is compatible with the hypothesis that the highest energy particles originate from nearby extragalactic sources whose flux has not been substantially reduced by interaction with the cosmic background radiation. AGN or objects having a similar…

Active galactic nucleus[SDU.ASTR.CO]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]AstronomyAstrophysics::High Energy Astrophysical Phenomenaparticle source [cosmic radiation]Cosmic background radiationFOS: Physical sciencesFluxOsservatorio Pierre AugerCosmic rayanisotropyAstrophysicsAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciences[PHYS.ASTR.CO]Physics [physics]/Astrophysics [astro-ph]/Cosmology and Extra-Galactic Astrophysics [astro-ph.CO]Raggi cosmici0103 physical sciencesUltra-high-energy cosmic ray010303 astronomy & astrophysicsBackground radiationNuclei galattivi attiviPhysicsPierre Auger ObservatorySPECTRUMMultidisciplinary[SDU.ASTR]Sciences of the Universe [physics]/Astrophysics [astro-ph]010308 nuclear & particles physicsMedicine (all); MultidisciplinaryMedicine (all)Settore FIS/01 - Fisica SperimentaleAstrophysics (astro-ph)angular dependence [cosmic radiation]Astrophysics::Instrumentation and Methods for AstrophysicsFísicaEnergia ultra altaExperimental High Energy Physicsddc:500Energy (signal processing)experimental results
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Long-term monitoring of mrk 501 for its very high energy γ emission and a flare in 2011 october

2012

"As one of the brightest active blazars in both X-ray and very high energy γ -ray bands, Mrk 501, is very useful for" "physics associated with jets from active galactic nuclei. The ARGO-YBJ experiment has monitored Mrk 501 for γ - rays above 0.3 TeV since 2007 November. The largest flare since 2005 was observed from 2011 October and lasted until about 2012 April. In this paper, a detailed analysis of this event is reported. During the brightest γ -ray flaring episodes from 2011 October 17 to November 22, an excess of the event rate over 6σ is detected by ARGO-YBJ in the direction of Mrk 501, corresponding to an increase of the γ -ray flux above 1 TeV by a factor of 6.6 ± 2.2 from its steady…

Active galactic nucleusactive" ["galaxies]Astrophysics::High Energy Astrophysical PhenomenaFluxAstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics7. Clean energy01 natural sciencesSpectral linelaw.inventionlaw0103 physical sciencesBlazar010303 astronomy & astrophysicsPhysicsindividual (Markarian 501) – galaxies: active – gamma rays: general – radiation mechanisms: non-thermal [BL Lacertae objects]" "general" ["gamma rays]010308 nuclear & particles physicsBL Lacertae objects: individual (Markarian 501) – galaxies: active – gamma rays: general – radiation mechanisms: non-thermalSettore FIS/01 - Fisica SperimentaleAstronomy and AstrophysicsQuasarGalaxyindividual (Markarian 501)" ["BL Lacertae objects]13. Climate actionSpace and Planetary ScienceSpectral energy distributionFlare
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Dissipative Processes and Their Role in the Evolution of Radio Galaxies

2019

Particle acceleration in relativistic jets to very high energies occurs at the expense of the dissipation of magnetic or kinetic energy. Therefore, understanding the processes that can trigger this dissipation is key to the characterization of the energy budgets and particle acceleration mechanisms at action in active galaxies. Instabilities and entrainment are two obvious candidates to trigger dissipation. On the one hand, supersonic, relativistic flows threaded by helical fields, as expected from the standard formation models of jets in supermassive black-holes, are unstable to a series of magnetohydrodynamical instabilities, such as the Kelvin-Helmholtz, current-driven, or possibly the p…

Active galactic nucleuslcsh:AstronomyRadio galaxyAstrophysics::High Energy Astrophysical Phenomenagalaxies: activeFOS: Physical sciencesKinetic energy01 natural scienceslcsh:QB1-991X-rays: binariesAstrophysical jet0103 physical sciencesrelativistic processes ISM: jets and outflows010303 astronomy & astrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsJet (fluid)010308 nuclear & particles physicsAstronomy and AstrophysicsMechanicsgalaxies: jetsradiation mechanisms: non-thermalDissipationAstrophysics - Astrophysics of GalaxiesParticle accelerationAstrophysics of Galaxies (astro-ph.GA)MagnetohydrodynamicsAstrophysics - High Energy Astrophysical PhenomenamagnetohydrodynamicsGalaxies
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REM near-IR and optical multiband observations of PKS 2155-304 in 2005 : Erratum

2007

Fernandez Soto, Alberto, Alberto.Fernandez@uv.es

Active galaxies ; BL Lacertae objects ; Individual ; PKS 2155-30 ; Errata ; AddendaAddendaErrataActive galaxiesBL Lacertae objectsIndividualPKS 2155-30UNESCO::ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogoniaUNESCO::ASTRONOMÍA Y ASTROFÍSICA:ASTRONOMÍA Y ASTROFÍSICA::Cosmología y cosmogonia [UNESCO]:ASTRONOMÍA Y ASTROFÍSICA [UNESCO]
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Evaluation of Antimicrobial Activity of Triphala Constituents and Nanoformulation

2020

The prevalence of nosocomial infections due to multidrug resistant (MDR) bacterial strains is associated with high morbidity and mortality. Folk medicine and ethnopharmacological data can provide a broad range of plants with promising antimicrobial activity. Triphala, an Ayurvedic formula composed of three different plants: Terminalia chebula Retz., Terminalia bellirica (Gaertn.) Roxb. (Combretaceae), and Phyllanthus emblica L. (Phyllanthaceae), is used widely for various microbial infections. Various extraction techniques were applied in the extraction of the biologically active constituents of Triphala in order to compare their efficiency. Microwave-assisted extraction (MAE) was shown to …

Active ingredient0303 health sciencesTraditional medicineArticle SubjectCetyl alcoholAntimicrobial01 natural sciencesDosage form0104 chemical sciencesTerminalia chebulaOther systems of medicine010404 medicinal & biomolecular chemistry03 medical and health scienceschemistry.chemical_compoundIngredientComplementary and alternative medicinechemistryCarvacrolTriphalaRZ201-999Research Article030304 developmental biologyEvidence-Based Complementary and Alternative Medicine
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Studies on the Effect of Cell Division-inhibiting Herbicides on Unialgal and Mixed Algal Cultures

1989

The effect of two cell division inhibiting herbicides on unialgal and mixed algal cultures was studied in laboratory tests. The herbicides studied were trifluralin (analytical grade) and the active ingredient as well as the preparation (80 % a.i.) of diphenamid. The three green algal species used were Selenastrum capricornutum PRINTZ, Scenedesmus quadricauda (TURP.) BREB., Oocystis parva W. et G. S. WEST. The response of algae to herbicides was determined by cell counting, and measured by turbidity (750 nm) and the 02-production of some of the treated cultures. The EC50-value (96 h) of trifluralin to Selenastrum capricornutum was 3.3 mg/l. There were differences in the sensitivity of the th…

Active ingredientCell divisionbiologyTrifluralinSelenastrumAquatic Sciencebiology.organism_classificationCell countingchemistry.chemical_compoundchemistryAlgaeBotanyFood scienceGeneral Agricultural and Biological SciencesOocystisEcology Evolution Behavior and SystematicsScenedesmusInternationale Revue der gesamten Hydrobiologie und Hydrographie
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Application of LA-ICP-MS as a rapid tool for analysis of elemental impurities in active pharmaceutical ingredients.

2014

The control of inorganic contaminants in active pharmaceutical ingredients has a significant role in the quality control of drug products. The concentration limits for metal residues in drug products have been defined by various regulatory guidelines. Laser ablation inductively coupled plasma mass spectrometry (LA-ICP-MS) is a powerful and fast analytical technique for multi-elemental analysis. A disadvantage in using LA-ICP-MS method is the lack of matrix reference materials for validation and calibration purposes. This article focuses on the handling strategy of laboratory-made matrix calibration standards for the quantification of elemental impurities in an active pharmaceutical ingredie…

Active ingredientChromatographyChemistryLaser ablation inductively coupled plasma mass spectrometryClinical BiochemistryAnalytical techniqueAnalytical chemistryPharmaceutical ScienceAnalytical ChemistryMatrix (chemical analysis)Pharmaceutical PreparationsLa icp msSpectrometry Mass Matrix-Assisted Laser Desorption-IonizationDrug DiscoveryCalibrationInorganic contaminantsElemental impuritiesDrug ContaminationSpectroscopyJournal of pharmaceutical and biomedical analysis
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Trehalose-hydroxyethylcellulose microspheres containing vancomycin for topical drug delivery.

2001

Abstract A new formulation, in which vancomycin is entrapped into trehalose and hydroxyethylcellulose (Natrosol ® ) spherical matrices, is described. Microspheres were produced by the solvent evaporation method. The entrapped drug was fully recovered following microspheres dissolution. Differential scanning calorimetry analyses proved that Natrosol maintains trehalose in its amorphous form. The stabilizing effects of trehalose on vancomycin were evaluated even after long storage and heating of microspheres. Calorimetric data indicated no decomposition of the entrapped drug. In vitro drug release, already performed by using a general two-compartment linear time-invariant open model, suggests…

Active ingredientChromatographyChemistryStereochemistryPharmaceutical ScienceTrehaloseGeneral MedicineTrehaloseDosage formMicrospheresAnti-Bacterial Agentschemistry.chemical_compoundDifferential scanning calorimetryDrug Delivery SystemsSolubilityVancomycinLiberationDrug carrierCelluloseDissolutionBiotechnologyAntibacterial agentEuropean journal of pharmaceutics and biopharmaceutics : official journal of Arbeitsgemeinschaft fur Pharmazeutische Verfahrenstechnik e.V
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