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From Centimeter to Millimeter Wavelengths: A High Angular Resolution Study of 3C273
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🌌 astro-ph
keywords
c273angularbandsbasecentimetercomponentdiscusseffects
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We monitored 3C273 with VLBI at 15-86 GHz since 1990. We discuss component trajectories, opacity effects at the jet base, a rotating and perhaps precessing jet, and outburst-ejection relations from Gamma-ray to radio bands.
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