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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

Inlists used for the creation of initial models as well as for flashing/stably burning models.

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technical details

MESA version(s) used and other details.

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Steadily 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.

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