Image Details
Caption: Figure 7.
Same as Figure 6, shown for the SG model on a uniform logarithmic grid with models separated by a factor of 2. In the parameters indicated by gray circles in the lower left and upper right regions, BHs with mBH = 50 M⊙ remain in the ADIOS and ZEBRA states, respectively, irrespective of kicks.
© 2026. The Author(s). Published by the American Astronomical Society.