[Mesa-users] mesa r10398, suite-case make_co_wd, question about inlist

Александр Сергеевич Андрюшин andriushin.as14 at physics.msu.ru
Mon Mar 11 05:13:32 EDT 2019


>
> Thank you, Francis, for your concern.. I ve managed to evolve a 2.99 msun
> model from pre-ms to wd (without using make-co-wd suitecase) ..
> But i have not succeeded much yet with evolving 5 msun model to wd though
> i' ve experimented with varcontrol and mesh_delta coefficient.. It seems
> that my prepare_to_make_co_wd_inlist lacks some stop-evolving condition
> (even on the planetary nebula stage, with no envelope remained, the model
> is being evolved with this inlist , not with make_co_wd_inlist ... while
> the following work of yours https://arxiv.org/abs/1301.0319 (p.12) made
> me think that in case of 5 msun the model evolving with make_co_wd_inlist
> is being started with post-AGB, where the thermal pulses are halted
> because envelope is lost very quickly).. Probably, i m wrong to use the
> mentioned suitecase, because what i need in my work is not only the wd
> masses for different initial star masses, but also massloss rates closer to
> realistic..
>
> On Mar 10, 2019, at 2:58 PM, Francis Timmes via Mesa-users <
> mesa-users at lists.mesastar.org> wrote:
>
> hi alex,
>
> to perhaps help move you along ...
>
> attached is a mesa work directory that evolves a 2.1 msun model from the
> pre-ms to a wd.
> this is from one of my ongoing active science projects, which saw its
> opening salvo in https://ui.adsabs.harvard.edu/#abs/2018ApJ...867L..30T/
> abstract . i also used a variation
> of this work directory in the 2018 mesa summer school (
> http://cococubed.asu.edu/mesa_market/education.html).
>
> the inlist_project uses the new convective pre-mixing described in the
> mesa V instrument paper,
> https://ui.adsabs.harvard.edu/?#abs/2019arXiv190301426P/abstract , and
> the model results will
> probably get very close to the evolutionary track shown in figure 1.
>
> fxt
>
>
>
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