[mesa-users] 2Msun to RGB tip model

[Bill Wolf]

Replying to get this back on mesa-users. Sorry about that.

Regards,

Bill
On October 19, 2016 at 6:14:56 PM, trobolo dinni (trobolo.trobolo.dinni5 at gmail.com) wrote:

Hi Bill,

thanks for the suggestion, I will try that as a start and see what the model output is. 

Concerning the stop time, I could simply check when the RGB tip happens (approximately) and rerun the simulation with that as a stop time. This is very brutal but what I am in need of are a couple of profiles around the RGB tip to use as a start for a 3D hydro simulation. It is just a test at this stage.

Regards,
Roberto




On 20 October 2016 at 11:59, Bill Wolf <wmwolf at physics.ucsb.edu> wrote:
Hi Roberto,

Your requirements are very vague, so many test cases may suit your requirements. My first choice would be the 1M_pre_ms_to_wd, setting the initial mass to 2 instead of 1. You'll need to figure out how to stop evolution at the RGB tip, though.

Regards,

Bill

On Wed, Oct 19, 2016 at 5:47 PM, trobolo dinni <trobolo.trobolo.dinni5 at gmail.com> wrote:
Dear MESA users,

I want to run a stellar model from pre-main sequence to the RGB tip (initial mass 2Msun) without any particular specifics, very simple. The most standard parameters.

I would like to ask what would be a good test suite model to start from or what set of main parameters would you suggest.

Best regards,
Roberto 

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