[Mesa-users] Problems with post-AGB track

[Janis Rodríguez]

Hi everyone,

I've been working with evolution models of low-mass stars, some of them
have experienced a very late thermal pulse (VLTP). When these models return
through the post-AGB trace, they begin to increase their luminosity instead
of remaining constant, as shown in the figure attached to the email. I've
noticed that in these cases the He luminosity  is greater than the first
time it passed through this trace, as shown in the video. I tried to
restrict the changes in the He luminosity  but it has not worked. Do you
have an idea how I can keep the brightness constant?

Thanks,
Janis
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