Evidence for Two Distinct Broad-line Regions from Reverberation Mapping of PG 0026+129
Chen Hu, Sha-Sha Li, Wei-Jian Guo, Sen Yang, Zi-Xu Yang, Dong-Wei Bao, Bo-Wei Jiang, Pu Du, Yan-Rong Li, Ming Xiao, Yu-Yang Songsheng, Zhe Yu, Jin-Ming Bai, Luis C. Ho, Wei-Hao Bian, Michael S. Brotherton, Ye-Fei Yuan, Jesús Aceituno, Hartmut Winkler, Jian-Min Wang
Abstract
Abstract We report on the results of a new spectroscopic monitoring campaign of the quasar PG 0026+129 at the Calar Alto Observatory 2.2 m telescope from 2017 July to 2020 February. Significant variations in the fluxes of the continuum and broad emission lines, including H β and He ii , were observed in the first and third years, and clear time lags between them are measured. The broad H β line profile consists of two Gaussian components: an intermediate-width H with an FWHM of 1964 ± 18 and another very broad H with an FWHM of 7570 ± 83 . H has long time lags of ∼40–60 days in the rest frame, while H shows nearly zero time delay with respect to the optical continuum at 5100 Å. The velocity-resolved delays show consistent results: lags of ∼30–50 days at the core of the broad H β line and roughly zero lags at the wings. H has a redshift of ∼400 , which seems to be stable for nearly 30 yr by comparing with archived spectra, and may originate from an infall. The rms spectrum of H shows a double-peaked profile with brighter blue peak and extended red wing in the first year, which matches the signature of a thin disk. Both the double-peaked profile and the near-zero lag suggest that H comes from a region associated with the part of the accretion disk that emits the optical continuum. Adopting the FWHM (in the rms spectrum) and the time lag measured for the total H β line, and a virial factor of 1.5, we obtain a virial mass of for the central black hole in this quasar.