[mesa-users] MESA3 paper massive binary example

[Pablo Marchant]

Roni, together with the inlists there is a run_star_extras.f provided (and
in the inlists it is said that you need it). Are you using it? From you
output it seems not. This implements the switch from a Kudritski wind to a
Hamann one as described in Wellstein & Langer 1999.

I guess changing this will make it consistent with that of the paper. Your
model is doing some crazy things though.

On Mon, Jun 15, 2015 at 9:06 AM, Roni Waldman <roni181066 at gmail.com> wrote:

> Hi Pablo,
> Too big for one email, will send several.
> Thanks,
> Roni
>
> ‫בתאריך יום א׳, 14 ביוני 2015 ב-22:55 מאת ‪Pablo Marchant‬‏ <‪
> pamarca at gmail.com‬‏>:‬
>
>> Roni, can you send me your history.data for each star and
>> binary_history.data to compare?
>>
>> On Sun, Jun 14, 2015 at 8:35 PM, Roni Waldman <roni181066 at gmail.com>
>> wrote:
>>
>>> Hi,
>>>
>>> I downloaded the inlists of the MESA3 paper, and ran the example
>>> 6_massive_binary, without changing anything in the inlists or the code,
>>> version 7624.
>>> The run ends with the donor having 2Msun, the accretor filling its
>>> Roche-lobe, and the time steps being super small (1e-12).
>>> This not what seems to happen in the paper.
>>> Am I doing anything wrong?
>>>
>>> Roni
>>>
>>>
>>>
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>>
>>
>> --
>> Pablo Marchant Campos
>> M.Sc on Astrophysics, Universidad Católica de Chile
>> PhD student, Argelander-Institut für Astronomie
>>
>


-- 
Pablo Marchant Campos
M.Sc on Astrophysics, Universidad Católica de Chile
PhD student, Argelander-Institut für Astronomie
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