Search results for "galaxies: individual: 3C 111"

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VLBA polarimetric monitoring of 3C 111

2018

Context. While studies of large samples of jets of active galactic nuclei (AGN) are important in order to establish a global picture, dedicated single-source studies are an invaluable tool for probing crucial processes within jets on parsec scales. These processes involve in particular the formation and geometry of the jet magnetic field as well as the flow itself. Aims. We aim to better understand the dynamics within relativistic magneto-hydrodynamical flows in the extreme environment and close vicinity of supermassive black holes. Methods. We analyze the peculiar radio galaxy 3C 111, for which long-Term polarimetric observations are available. We make use of the high spatial resolution of…

active [Galaxies]Radio galaxyAstrophysics::High Energy Astrophysical PhenomenaeducationFOS: Physical sciencesAstrophysicsgalaxies [Radio continuum]Astrophysics::Cosmology and Extragalactic Astrophysics01 natural sciencesRadio continuum: galaxiesgalaxies: individual: 3C 111Coincident0103 physical sciences010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsPhysicsSupermassive black holepolarizationGalaxies: magnetic fields010308 nuclear & particles physicsmagnetic fields [Galaxies]Astronomy and AstrophysicsGalaxies: activePolarization (waves)Astrophysics - Astrophysics of GalaxiesMonitoring programMagnetic fieldTransverse planeindividual: 3C 111 [galaxies]Space and Planetary ScienceGalaxies: jetsBrightness temperatureAstrophysics of Galaxies (astro-ph.GA)jets [Galaxies]
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Sub-milliarcsecond imaging of a bright flare and ejection event in the extragalactic jet 3C 111

2020

Context. Flares in radio-loud active galactic nuclei are thought to be associated with the injection of fresh plasma into the compact jet base. Such flares are usually strongest and appear earlier at shorter radio wavelengths. Hence, very long baseline interferometry (VLBI) at millimeter(mm)-wavelengths is the best-suited technique for studying the earliest structural changes of compact jets associated with emission flares. Aims. We study the morphological changes of the parsec-scale jet in the nearby (z = 0.049) γ-ray bright radio galaxy 3C 111 following a flare that developed into a major radio outburst in 2007. Methods. We analyse three successive observations of 3C 111 at 86 GHz with th…

individual: 3C 111 [Galaxies]active [Galaxies]Astrophysics::High Energy Astrophysical PhenomenaFOS: Physical sciencesLibrary scienceAstrophysics::Cosmology and Extragalactic AstrophysicsAstrophysicsGalaxies: individual: 3C 1117. Clean energy01 natural sciencesTechniques: high angular resolutionObservatory0103 physical sciencesVery-long-baseline interferometryAstrophysics::Solar and Stellar Astrophysicsmedia_common.cataloged_instanceEuropean union010303 astronomy & astrophysicsAstrophysics::Galaxy AstrophysicsVery Long Baseline Arraymedia_commonHigh Energy Astrophysical Phenomena (astro-ph.HE)Physics010308 nuclear & particles physicsEuropean researchAstronomy and AstrophysicsGalaxies: activeMonitoring programRadio astronomy observatory3. Good healthhigh angular resolution [Techniques]Galaxies: jetsSpace and Planetary Sciencejets [Galaxies]Christian ministryAstrophysics - High Energy Astrophysical PhenomenaAstronomy & Astrophysics
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