The input files for "A Rare Population of Intermediate-mass Helium Stars Between Hot Subdwarfs and Wolf-Rayet Stars"

Core Evolution / Stellar Structure / Interactions & CE / Mass Loss & Supernovae / Metallicity & Utilities / Tools & Analysis bse.f: Reads input file: "evolve.in" and coordinates binary evolution simulation. evolv2.f: Central algorithm for binary interactions (RLOF, mass transfer, CE, SNe). star.f: Calculates evolutionary timescales and luminosities (Eggleton formulas). hrdiag.f: Computes current stellar physical parameters (L, R, T, core mass). corerd.f: Determines core radius for giant stars. mrenv.f: Estimates convective envelope parameters. comenv.f: Models common envelope physics and energy balance. mix.f: Handles evolution of merger/collision products. mlwind.f: Implements various stellar wind mass-loss prescriptions. kick.f: Computes supernova kick velocity and orbital dynamics adjustments. zcnsts.f: Initializes metallicity-dependent parameters. zfuncs.f: Collection of metallicity-dependent evolution helper functions. deltat.f: Dynamically determines adaptive timesteps. popbin.f: Population synthesis file (! core file). lambda.f: Scripts for processing common envelope lambda parameters across metallicities.