Explaining a rapidly fading star as a type II ILOT in a triple star system

Bear, Soker and Kashi 2022<br> ========================== The code follows 1M_pre_ms_to_wd example in test suite.<br> Prior to running this code we run 12Mo when we follow the example of 16_predictive_mix example for 12Mo.<br> We look when this star of 12Mo leaves the MS, the time taken is 1.46X10^7 years. The code is divided to 2 stages:<br> Stage A: up to 1.46X10^7 years when no other changes have been made to the example. We save the file produces at 1.46X10^7years. Stage B: We restart the file at 1.46X10^7years and insert mass loss by enabling mass_change. The mass parameter for stage A+B is: 0.3Mo and 0.5Mo.<br> The mass_change parameter is 0.3X10^-5, 1X10^-5, 3X10^-5 Mo/yr Each stage contains the inlist and the data files used in https://arxiv.org/abs/2202.08629