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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
Exploring the magnetic field configuration close to central engines
Speakers
- Dr. Bindu RANI
Primary authors
- Dr. Bindu RANI (MPI für Radioastronomie)
Co-authors
- Dr. Thomas KRICHBAUM (MPI für Radioastronomie)
- Dr. Jeffrey HODGSON (MPI für Radioastronomie)
- Dr. Shoko KOYAMA (MPI für Radioastronomie)
- Prof. J. Anton ZENSUS (MPI für Radioastronomie)
- Prof. Alan MARSCHER (Boston University)
- Dr. Svetlana JORSTAD (Boston University)
Content
The high radio frequency polarization imaging of non-thermal emission from AGN is a direct way to probe the magnetic field strength and structure in the immediate vicinity of SMBHs and is crucial in testing the jet-launching scenario. To explore the the magnetic field configuration at the base of jets in blazars, I took advantage of the full polarization capabilities of the GMVA (Global Millimeter VLBI Array). With an angular resolution of ∼50μas, one could reach scales down to $\sim 720\,R_s$ (for a 10$^9$ solar mass black hole). In this talk, I will show the preliminary results of our study on BL Lac.
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