Reverberation Mapping of Changing-look Active Galactic Nucleus NGC 3516
arXiv:2012.15572 · doi:10.3847/1538-4357/abd851
Abstract
The changes of broad emission lines should be a crucial issue to understanding the physical properties of changing-look active galactic nucleus (CL-AGN). Here, we present the results of an intensive and homogeneous 6-month long reverberation mapping (RM) monitoring campaign during a low-activity state of the CL-AGN Seyfert galaxy NGC 3516. Photometric and spectroscopic monitoring was carried out during 2018--2019 with the Lijiang 2.4 m telescope. The sampling is 2 days in most nights, and the average sampling is 3 days. The rest frame time lags of H and H are days and days, respectively. From a RMS H line dispersion of and a virial factor of = 5.5, the central black hole mass of NGC 3516 is estimated to be , which is in agreement with previous estimates. The velocity-resolved delays show that the time lags increase towards negative velocity for both H and H. The velocity-resolved RM of H is done for the first time. These RM results are consistent with other observations before the spectral type change, indicating a basically constant BLR structure during the changing-look process. The CL model of changes of accretion rate seems to be favored by long-term H variability and RM observations of NGC 3516.
25 pages, 6 figures, Accepted for publication in ApJ
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