Monitoring AGNs with H{beta} Asymmetry. II.

All three of these targets have shown asymmetric broad H{beta} emission lines in the past, although their emission lines were relatively symmetric during our observations. We measured H{beta} time lags for all three targets and estimated masses of their black holes-for the first time in the case of Mrk 841.

For Mrk 79 and NGC 3227, the data are of sufficient quality to resolve distinct time lags as a function of velocity and to compute two-dimensional velocity-delay maps. Mrk 79 shows smaller time lags for high-velocity gas, but the distribution is not symmetric, and its complex velocity-delay map could result from the combination of both inflowing and outflowing H{beta} emitting disks that may be part of a single larger structure.