Millimeter VLBI of NGC 1052: Dynamics
AbstractThe LINER galaxy NGC 1052 is an ideal target to study the innermost regions of active galactic nuclei (AGN), given its close distance of about 20 Mpc. The source was observed at 29 epochs from 2005 to 2009 with the Very Long Baseline Array (VLBA) at 43 GHz. Here, we present a kinematic study of its twin-jet system from a subset of 9 epochs at 43 GHz carried out in 2005 and 2006, finding a bright central feature as the dynamic center. The resulting mean velocities of
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Baczko, A.-K.; Schulz, R.; Ros, E.; Kadler, M.; Perucho, M.; Wilms, J. Millimeter VLBI of NGC 1052: Dynamics. Galaxies 2016, 4, 48.
Baczko A-K, Schulz R, Ros E, Kadler M, Perucho M, Wilms J. Millimeter VLBI of NGC 1052: Dynamics. Galaxies. 2016; 4(4):48.Chicago/Turabian Style
Baczko, Anne-Kathrin; Schulz, Robert; Ros, Eduardo; Kadler, Matthias; Perucho, Manel; Wilms, Jörn. 2016. "Millimeter VLBI of NGC 1052: Dynamics." Galaxies 4, no. 4: 48.
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