Image Details
Caption: Figure 8.
Peak temperature (T p ) of the accretion disk model as a function of days since the UV/optical peak. Only sources with at least two fittable spectra and with no corona emission (see Section 4.3) are shown. The solid black line shows the expected theoretical evolution for a finite stress at the ISCO.
© 2024. The Author(s). Published by the American Astronomical Society.