Search results for "Radio astronomy observatory"

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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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