Image Details
Caption: Figure 5.
The temporal variations of Hβ and Hγ VRLPs are systematically compared across six observing seasons (2015, 2018, 2019, 2020, 2021, and 2023) using 30 equal-flux velocity bins, with lags below a maximum correlation coefficient of 0.5 excluded. Vertical and horizontal dotted lines indicate the line core at zero velocity and zero time lag, respectively.
© 2025. The Author(s). Published by the American Astronomical Society.