[Mesa-users] Question

[Nicholas Herrington]

Hello

I am new to MESA and have been running some models of very low metallicity
stars, accreting matter at very high rates. These stars become supermassive
very quickly, matching results from other stellar evolution codes we've
tried. At the current masses achieved, the stars should be on the verge of
collapse. I understand MESA has an implicit hydrodynamics solver. Long
story short, is this capability triggered throughout the evolution, given
the right conditions, or do I need to trigger this through a set of
controls in my inlist file.

I am using mesa-r12115 and mesa-r11701

Thank you for your time
Nick
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