Broad-line Region of the Quasar PG 2130+099 from a Two-year Reverberation Mapping Campaign with High Cadence
Chen Hu, Yanrong Li, Pu Du, Zhi-Xiang Zhang, Shasha Li, Ying-Ke Huang, Kai-Xing Lu, Jin-Ming Bai, Luis C. Ho, Wei‐Hao Bian, M. S. Brotherton, Ye‐Fei Yuan, J. Aceituno, Hartmut Winkler, Jian-Min Wang
Abstract
Abstract As one of the most interesting Seyfert 1 galaxies, PG 2130+099 has been the target of several reverberation mapping (RM) campaigns over the years. However, its measured broad H β line responses have been inconsistent, with time lags of ∼200 days, ∼25 days, and ∼10 days being reported for different epochs while its optical luminosity changed no more than 40%. To investigate this issue, we conducted a new RM-campaign with homogenous and high cadence (about ∼3 days) for two years during 2017–2019 to measure the kinematics and structure of the ionized gas. We successfully detected time lags of broad H β , He ii , He i , and Fe ii lines with respect to the varying 5100 Å continuum, revealing a stratified structure that is likely virialized with Keplerian kinematics in the first year of observations, but an inflow kinematics of the broad-line region from the second year. With a central black hole mass of , PG 2130+099 has an accretion rate of , where L Edd is the Eddington luminosity and c is speed of light, implying that it is a super-Eddington accretor and likely possesses a slim, rather than thin, accretion disk. The fast changes of the ionization structures of the three broad lines remain puzzling.