论文标题

用H $β$不对称监测AGN。 iii。 15个palomar绿色类星体的长期混响映射结果

Monitoring AGNs with H$β$ Asymmetry. III. Long-term Reverberation Mapping Results of 15 Palomar-Green Quasars

论文作者

Bao, Dong-Wei, Brotherton, Michael S., Du, Pu, McLane, Jacob N., Zastrocky, T. E., Olson, Kianna A., Fang, Feng-Na, Zhai, Shuo, Huang, Zheng-Peng, Wang, Kai, Zhao, Bi-Xuan, Li, Sha-Sha, Yang, Sen, Chen, Yong-Jie, Liu, Jun-Rong, Yao, Zhu-Heng, Peng, Yue-Chang, Guo, Wei-Jian, Songsheng, Yu-Yang, Li, Yan-Rong, Jiang, Bo-Wei, Kasper, David H., Chick, William T., Nguyen, My L., Maithil, Jaya, Kobulnicky, H. A., Dale, D. A., Hand, Derek, Adelman, C., Carter, Z., Murphree, A. M., Oeur, M., Schonsberg, S., Roth, T., Winkler, Hartmut, Marziani, Paola, D'Onofrio, Mauro, Hu, Chen, Xiao, Ming, Xue, Suijian, Czerny, Bożena, Aceituno, Jesús, Ho, Luis C., Bai, Jin-Ming, Wang, Jian-Min

论文摘要

在该系列报道的第三篇论文中,关于具有不对称的H $β$发射线轮廓的主动银河系核的混响映射(RM)活动,我们在2016年5月底至2021年5月底获得的光谱为15个Palomar-Green(PG)类星体提供了15个palomar-Green(PG)类星体的结果。该活动结合了长时间的跨度Spans与相对高高的固定性结合。对于8个对象,从整个光曲线中获得的两个时间滞后以及来自单个观察季节的测量值。我们的9个目标的混响映射是第一次尝试,而其他6个目标的结果可以与以前的广告系列进行比较。我们在几年内测量H $β$时间滞后,并估计其黑洞质量。该活动的漫长持续时间使我们能够通过使用速度分辨的滞后来研究不同年份的宽线区域(BLR)几何学和运动学,这表明了不同的BLR几何形状和运动学的特征。讨论了单个对象的BLR几何形状和运动学。在此样本中,开普勒/病毒运动和流入的BLR运动学比流出更常见。

In this third paper of the series reporting on the reverberation mapping (RM) campaign of active galactic nuclei with asymmetric H$β$ emission-line profiles, we present results for 15 Palomar-Green (PG) quasars using spectra obtained between the end of 2016 to May 2021. This campaign combines long time spans with relatively high cadence. For 8 objects, both the time lags obtained from the entire light curves and the measurements from individual observing seasons are provided. Reverberation mapping of 9 of our targets has been attempted for the first time, while the results for 6 others can be compared with previous campaigns. We measure the H$β$ time lags over periods of years and estimate their black hole masses. The long duration of the campaign enables us to investigate their broad line region (BLR) geometry and kinematics for different years by using velocity-resolved lags, which demonstrate signatures of diverse BLR geometry and kinematics. The BLR geometry and kinematics of individual objects are discussed. In this sample, the BLR kinematics of Keplerian/virialized motion and inflow is more common than outflow.

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