Stellar mass (left panels) and cooling times (right panels) vs. log g and log T_eff for post-CE non-flashing sequences with minimum M_H (no H burning; top) and maximum M_H (H burning; bottom). Green symbols mark CE He WDs (P<0.1 day) (Brown et al. 2020). Sequences with H burning show much longer cooling times, exceeding several Gyr at low log T_eff, while those with minimum M_H remain below 1 Gyr. In both cases, adjustment times after CE remain under 0.1 Myr.