Broad-line Region of the Quasar PG 2130+099. II. Doubling the Size Over Four Years?
Zhu-Heng Yao, Sen Yang, Wei-Jian Guo, Yong-Jie Chen, Yu-Yang, Songsheng, Dong-Wei Bao, Bo-Wei Jiang, Yi-Lin Wang, Hao Zhang, Chen Hu,, Yan-Rong Li, Pu Du, Ming Xiao, Jin-Ming Bai, Luis C. Ho, Michael S., Brotherton, Jes\'us Aceituno, Hartmut Winkler, Jian-Min Wang

TL;DR
This study extends reverberation mapping of quasar PG 2130+099 over four years, revealing a doubling of the broad-line region size and complex dynamics, challenging previous inconsistent measurements and suggesting geometric dilution effects.
Contribution
It provides the first long-term, high-cadence monitoring of PG 2130+099, demonstrating significant BLR size variation and complex velocity-resolved delays, advancing understanding of quasar BLR dynamics.
Findings
Hβ lag increased by a factor of two in two years
Velocity delays show virial motion and inflow signs
Significant scatter in R-L relationship due to size changes
Abstract
Over the past three decades, multiple reverberation mapping (RM) campaigns conducted for the quasar PG 2130+099 have exhibited inconsistent findings with time delays ranging from 10 to 200 days. To achieve a comprehensive understanding of the geometry and dynamics of the broad-line region (BLR) in PG 2130+099, we continued an ongoing high-cadence RM monitoring campaign using the Calar Alto Observatory 2.2m optical telescope for an extra four years from 2019 to 2022. We measured the time lags of several broad emission lines (including He II, He I, H, and Fe II) with respect to the 5100 {\AA} continuum, and their time lags continuously vary through the years. Especially, the H time lags exhibited approximately a factor of two increase in the last two years. Additionally, the velocity-resolved time delays of the broad H emission line reveal a back-and-forth…
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Taxonomy
TopicsGalaxies: Formation, Evolution, Phenomena · Astronomy and Astrophysical Research · Geophysics and Gravity Measurements
