2021ApJ...920..112B

We have modeled the full velocity-resolved reverberation response of the Hβ and He II optical broad emission lines in NGC 3783 to constrain the geometry and kinematics of the low-ionization and high-ionization broad-line region (BLR). The geometry is found to be a thick disk that is nearly face-on, inclined at ∼18° to our line of sight, and exhibiting clear ionization stratification, with an extended Hβ-emitting region (r_median=10.07_–1.12^+1.10 lt-day) and a more compact and centrally located He II-emitting region (r_median=1.33_–0.42^=+0.34 lt-day). In the Hβ-emitting region, the kinematics are dominated by near-circular Keplerian orbits, but with ∼40% of the orbits inflowing. The more compact He II-emitting region, on the other hand, appears to be dominated by outflowing orbits. The black hole mass is constrained to be M_BH = 2.82_–0.63^+1.55×10⁷M_☉, which is consistent with the simple reverberation constraint on the mass based on a mean time delay, line width, and scale factor of <f> = 4.82. The difference in kinematics between the Hβ- and He II-emitting regions of the BLR is intriguing given the recent history of large changes in the ionizing luminosity of NGC 3783 and evidence for possible changes in the BLR structure as a result.