Hydrogen Burning on Accreting White Dwarfs: Stability, Recurrent Novae, and the Post-Nova Supersoft Phase
Inlists, model, and technical information for MESA simulations presented in
Wolf, Bildsten, Brooks & Paxton. 2013, ApJ, 777, 136
Inlists used for the creation of initial models as well as for flashing/stably burning models.
Saved models doing steady hydrogen burning. All have a tau_factor of 30 and a current network of 'cno_extras_o18_to_mg26_plus_fe56.net'. Velocities are on, but rotation is off.
Steadily Burning Models -