[Mesa-users] How is defined the upper limit of the star core?

anne.thoul at uliege.be anne.thoul at uliege.be
Sun Sep 16 04:49:07 EDT 2018


Hi Roque,

I am not sure what you mean by « star core » and « outermost limit of the center ».

In the history file you can for example decide to have the mass of the convective core  mass_conv_core (provided the star has a convective core). 
There is also the he_core_mass. 

For the exact definition of these quantities, you can proceed like Bill explained.

I hope this helps

Anne


> Le 16 sept. 2018 à 00:30, Roque Caballero Navarro via Mesa-users <mesa-users at lists.mesastar.org> a écrit :
> 
> Hi there,
> 
>    How is defined the upper limit of the star core? For example, I'm 
> using the following stop condition for finishing the simulation where 
> the TAMS is reached:
> 
>       ! stop when the center mass fraction of h1 drops below this limit
>       xa_central_lower_limit_species(1) = 'h1'
>       xa_central_lower_limit(1) = 1d-9
> 
> Which condition determines the outermost limit of the center?
> 
> Kind regards,
> 
> Roque
> 
> _______________________________________________
> mesa-users at lists.mesastar.org
> https://lists.mesastar.org/mailman/listinfo/mesa-users
> 

-------------- next part --------------
An HTML attachment was scrubbed...
URL: <https://lists.mesastar.org/pipermail/mesa-users/attachments/20180916/2ebe53c7/attachment.html>


More information about the Mesa-users mailing list