A Reverberation-Based Black Hole Mass for MCG-06-30-15
arXiv:1608.01229 · doi:10.3847/0004-637X/830/2/136
Abstract
We present the results of a reverberation campaign targeting MGC-06-30-15. Spectrophotometric monitoring and broad-band photometric monitoring over the course of 4 months in the spring of 2012 allowed a determination of a time delay in the broad H emission line of days in the rest frame of the AGN. Combined with the width of the variable portion of the emission line, we determine a black hole mass of M. Both the H time delay and the black hole mass are in good agreement with expectations from the - and relationships for other reverberation-mapped AGNs. The H time delay is also in good agreement with the relationship between H and broad-band near-IR delays, in which the effective BLR size is times smaller than the inner edge of the dust torus. Additionally, the reverberation-based mass is in good agreement with estimates from the X-ray power spectral density break scaling relationship, and with constraints based on stellar kinematics derived from integral field spectroscopy of the inner kpc of the galaxy.
13 pages, 9 figures, 4 tables, accepted for publication in ApJ
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