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from 30 November 2015 to 2 December 2015
Max-Planck-Institut für Radioastronomie, Bonn, Germany
Europe/Berlin timezone
Contribution Contributed
Max-Planck-Institut für Radioastronomie, Bonn, Germany
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0.02
mm-VLBI Observations of the Active Galaxy 3C 111 in Outburst
Speakers
- Mr. Robert SCHULZ
Primary authors
- Mr. Robert SCHULZ (Univ. Erlangen-Nürnberg; Univ. Würzburg)
Co-authors
- Prof. Matthias KADLER (Univ. Würzburg)
- Prof. Eduardo ROS (MPI für Radioastronomie & Univ. València)
- Dr. Thomas P. KRICHBAUM (MPI für Radioastronomie)
- Dr. Christoph GROßBERGER (MPI für extraterrestrische Physik)
- Dr. Cornelia MÜLLER (Radboud University)
- Prof. Karl MANNHEIM (Univ. Würzburg)
- Dr. Iván AGUDO (Instituto de Astrofísica de Andalucía - CSIC)
- Dr. Hugh D. ALLER (University of Michigan)
- Prof. Margo F. ALLER (University of Michigan)
Content
In 2007, the nearby (z=0.049) broad line radio galaxy 3C 111 exhibited a major flux density outburst. Three GMVA millimetre-VLBI observations at 86 GHz covering one year were conducted and allow us to study this outburst with unprecedented image fidelity at highest resolution of ~0.050 mas (~0.05 pc). The outburst led to the appearance of a complex series of plasma components forming an intriguing bent structure, being ejected at varying position angles. Within 1 pc from the jet base, ejections vary in position angle and components move with an apparent velocity of ~3 - 4c, significantly slower than the maximum velocity observed with cm-VLBI on scales beyond 1 mas.
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