paper

Black hole mass measurement using ALMA observations of [CI] and CO emissions in the Seyfert 1 galaxy NGC7469

arXiv:2104.03539 · doi:10.1093/mnras/stab1002

Abstract

We present a supermassive black hole (SMBH) mass measurement in the Seyfert 1 galaxy NGC7469 using Atacama Large Millimeter/submillimeter Array (ALMA) observations of the atomic-(1-0) and molecular-CO(1-0) emission lines at the spatial resolution of " (or 100 pc). These emissions reveal that NGC7469 hosts a circumnuclear gas disc (CND) with a ring-like structure and a two-arm/bi-symmetric spiral pattern within it, surrounded by a starbursting ring. The CND has a relatively low (") and (), suggesting that the gas is dynamically settled and suitable for dynamically deriving the mass of its central source. As is expected from X-ray dominated region (XDR) effects that dramatically increase an atomic carbon abundance by dissociating CO molecules, we suggest that the atomic [CI](1-0) emission is a better probe of SMBH masses than CO emission in AGNs. Our dynamical model using the (1-0) kinematics yields a M and (M/L). The model using the CO(1-0) kinematics also gives a consistent with a larger uncertainty, up to an order of magnitude, i.e.\ M. This newly dynamical is 2 times higher than the mass determined from the reverberation mapped (RM) method using emissions arising in the unresolved broad-line region (BLR). Given this new , we are able to constrain the specific RM dimensionless scaling factor of for the AGN BLR in NGC7469. The gas within the unresolved BLR thus has a Keplerian virial velocity component and the inclination of , confirming its face-on orientation in a Seyfert 1 AGN by assuming a geometrically thin BLR model.

22 pages, 16 figures, 7 tables. Accepted for publication on MNRAS

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