inlists

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

inlist_flash

Typical inlist for modeling flashes or stable burning. This particular inlists models a 1.00 Msun WD accreting at 5.0e-7 Msun/yr. Both Super Eddington winds and Roche lobe overflow are turned on, but in the paper only one mass loss mechanism was allowed at a time. Places needing customization for different masses and/or accretion rates are indicated with comments.

inlist_flash — Octet Stream, 17 kB (17793 bytes)

inlist_co_nova_1

First inlist in accretion starting process.

inlist_co_nova_1 — Octet Stream, 6 kB (6615 bytes)

inlist_co_nova_2

Second inlist in accretion starting process.

inlist_co_nova_2 — Octet Stream, 5 kB (5912 bytes)

inlist_co_nova_3

Third inlist in accretion starting process.

inlist_co_nova_3 — Octet Stream, 7 kB (8033 bytes)

inlist_co_nova_4

Fourth inlist in accretion starting process.

inlist_co_nova_4 — Octet Stream, 6 kB (6927 bytes)