Search results for "PARTICLES"

showing 10 items of 8085 documents

Wind-luminosity evolution in NLS1 AGN 1H 0707−495

2021

Ultra-fast outflows (UFOs) have been detected in the high-quality X-ray spectra of a number of active galactic nuclei (AGN) with fairly high accretion rates and are thought to significantly contribute to the AGN feedback. After a decade of dedicated study, their launching mechanisms and structure are still not well understood, but variability techniques may provide useful constraints. In this work, therefore, we perform a flux-resolved X-ray spectroscopy on a highly accreting and variable NLS1 AGN, 1H 0707-495, using all archival XMM-Newton observations to study the structure of the UFO. We find that the wind spectral lines weaken at higher luminosities, most likely due to an increasing ion…

Active galactic nucleusAstrophysics::High Energy Astrophysical Phenomenablack hole physicsFOS: Physical sciencesAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysics01 natural sciencesSpectral lineLuminosityaccretionIonization0103 physical sciencesAstrophysics::Solar and Stellar AstrophysicsEmission spectrum010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsHigh Energy Astrophysical Phenomena (astro-ph.HE)PhysicsAccretion (meteorology)010308 nuclear & particles physicsAstronomy and AstrophysicsRadiusaccretion discsgalaxies: SeyfertSpace and Planetary ScienceX-rays: individual: 1H 0707−495OutflowAstrophysics - High Energy Astrophysical Phenomena[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]Monthly Notices of the Royal Astronomical Society
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The history of chemical enrichment in the intracluster medium from cosmological simulations

2017

The distribution of metals in the intracluster medium (ICM) of galaxy clusters provides valuable information on their formation and evolution, on the connection with the cosmic star formation and on the effects of different gas processes. By analyzing a sample of simulated galaxy clusters, we study the chemical enrichment of the ICM, its evolution, and its relation with the physical processes included in the simulation and with the thermal properties of the core. These simulations, consisting of re-simulations of 29 Lagrangian regions performed with an upgraded version of the SPH GADGET-3 code, have been run including two different sets of baryonic physics: one accounts for radiative coolin…

Active galactic nucleusCosmology and Nongalactic Astrophysics (astro-ph.CO)Radiative coolingGalaxies:clusters:general; Galaxies:clusters:Intracluster medium; Methods: numerical; Astronomy and Astrophysics; Space and Planetary ScienceMetallicityFOS: Physical sciencesclusters:Intracluster medium [Galaxies]AstrophysicsAstrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesSmoothed-particle hydrodynamicsclusters:general [Galaxies]Intracluster medium0103 physical sciencesGalaxies:clusters:Intracluster medium010303 astronomy & astrophysicsGalaxy clusterAstrophysics::Galaxy AstrophysicsPhysicsnumerical [Methods]Methods: numerical010308 nuclear & particles physicsStar formationAstronomyAstronomy and AstrophysicsAstronomy and AstrophysicAstrophysics - Astrophysics of GalaxiesGalaxies:clusters:generalSupernova13. Climate actionSpace and Planetary ScienceAstrophysics of Galaxies (astro-ph.GA)Astrophysics - Cosmology and Nongalactic Astrophysics
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Coupling hydrodynamics and radiation calculations for star-jet interactions in active galactic nuclei

2016

Context. Stars and their winds can contribute to the non-thermal emission in extragalactic jets. Because of the complexity of jet-star interactions, the properties of the resulting emission are closely linked to those of the emitting flows. Aims. We simulate the interaction between a stellar wind and a relativistic extragalactic jet and use the hydrodynamic results to compute the non-thermal emission under different conditions. Methods. We performed relativistic axisymmetric hydrodynamical simulations of a relativistic jet interacting with a supersonic, non-relativistic stellar wind. We computed the corresponding streamlines out of the simulation results and calculated the injection, evolut…

Active galactic nucleusElectromagnetic spectrumAstrophysics::High Energy Astrophysical PhenomenaAstrophysics::Cosmology and Extragalactic AstrophysicsElectronAstrophysicsRadiation7. Clean energy01 natural sciencessymbols.namesake0103 physical sciencesAstrophysics::Solar and Stellar Astrophysics010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsHidrodinàmica010308 nuclear & particles physicsAstronomy and AstrophysicsStarsEstelsMagnetic fieldParticle accelerationStars13. Climate actionSpace and Planetary ScienceHydrodynamicssymbolsDoppler effectAstronomy & Astrophysics
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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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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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Targeted-lung delivery of dexamethasone using gated mesoporous silica nanoparticles. A new therapeutic approach for acute lung injury treatment

2021

Acute lung injury (ALI) is a critical inflammatory syndrome, characterized by increased diffuse inflammation and severe lung damage, which represents a clinical concern due to the high morbidity and mortality in critical patients. In last years, there has been a need to develop more effective treatments for ALI, and targeted drug delivery to inflamed lungs has become an attractive research field. Here, we present a nanodevice based on mesoporous silica nanoparticles loaded with dexamethasone (a glucocorticoid extensively used for ALI treatment) and capped with a peptide that targets the TNFR1 receptor expressed in pro-inflammatory macrophages (TNFR-Dex-MSNs) and avoids cargo leakage. TNFR-D…

Acute Lung InjuryPharmaceutical ScienceInflammationLung injuryPharmacologyDexamethasoneMiceIn vivomedicineAnimalsHumansLungDexamethasoneLungbusiness.industryrespiratory systemSilicon Dioxiderespiratory tract diseasesmedicine.anatomical_structureTargeted drug deliveryNanoparticlesTumor necrosis factor alphamedicine.symptombusinessGlucocorticoidmedicine.drugJournal of Controlled Release
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Therapeutic Vaccination of Hematopoietic Cell Transplantation Recipients Improves Protective CD8 T-Cell Immunotherapy of Cytomegalovirus Infection

2021

Reactivation of latent cytomegalovirus (CMV) endangers the therapeutic success of hematopoietic cell transplantation (HCT) in tumor patients due to cytopathogenic virus spread that leads to organ manifestations of CMV disease, to interstitial pneumonia in particular. In cases of virus variants that are refractory to standard antiviral pharmacotherapy, immunotherapy by adoptive cell transfer (ACT) of virus-specific CD8+ T cells is the last resort to bridge the “protection gap” between hematoablative conditioning for HCT and endogenous reconstitution of antiviral immunity. We have used the well-established mouse model of CD8+ T-cell immunotherapy by ACT in a setting of experimental HCT and mu…

Adoptive cell transfermedicine.medical_treatmentImmunologyCytomegalovirusCD8-Positive T-LymphocytesLymphocyte ActivationCD8+ T cellsVirusCytomegalovirus VaccinesImmunocompromised HostAntigenvaccineMHC class ImedicineImmunology and AllergyCytotoxic T cellAnimalsCells Culturedadoptive cell transferCell ProliferationOriginal ResearchHCMV dense bodiesbiologybusiness.industryVaccinationHematopoietic Stem Cell TransplantationImmunotherapyRC581-607VirologyAdoptive TransferTransplantationMice Inbred C57BLantiviral protectionT cell primingDisease Models AnimalT cell receptor transgenic cellsCytomegalovirus InfectionsHost-Pathogen Interactionsbiology.proteinFemaleVirus Activationsubviral particlesImmunologic diseases. AllergybusinessCD8Frontiers in Immunology
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Circulating microparticles as disease-specific biomarkers of severity of inflammation in patients with hepatitis C or nonalcoholic steatohepatitis.

2012

Background & Aims Microparticles released into the bloodstream upon activation or apoptosis of CD4+ and CD8+ T cells correlate with inflammation as determined by histologic analysis in patients with chronic hepatitis C (CHC). Patients with nonalcoholic fatty liver (NAFL) or nonalcoholic steatohepatitis (NASH) can be differentiated from those with CHC based on activation of distinct sets of immune cells in the liver. Methods We compared profiles of circulating microparticles from patients with NAFL and NASH (n = 67) to those of CHC (n = 42), with healthy individuals (controls) using flow cytometry; the profiles were correlated with inflammation grade and fibrosis stage based on histologic an…

AdultCD4-Positive T-LymphocytesLiver CirrhosisMaleLymphocyteBiologyCD8-Positive T-LymphocytesChronic liver diseaseSeverity of Illness IndexArticleCell-Derived MicroparticlesDiagnosis DifferentialImmune systemFibrosisCell-Derived MicroparticlesNon-alcoholic Fatty Liver DiseasemedicineHumansAgedAged 80 and overInflammationHepatologyFatty liverBiopsy NeedleGastroenterologyAlanine TransaminaseHepatitis CHepatitis C ChronicMiddle Agedmedicine.diseaseFlow CytometryFatty Livermedicine.anatomical_structureAlanine transaminaseLiverROC CurveCase-Control StudiesImmunologybiology.proteinLinear ModelsFemaleBiomarkersGastroenterology
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