[mesa-users] jay

Martin C. martincs14 at gmail.com
Wed Jun 1 21:01:45 EDT 2016


Hi Pablo,
ok thanks.

Maybe this is somewhere on the website, but can't find it:
is the second mass (m2) in binaries always assumed to be the accretor?

This
accretor_overflow_terminate = 0.0d0
seems to affect the second mass.

thx,

Martin

On Wed, Jun 1, 2016 at 3:42 AM, Pablo Marchant <pamarca at gmail.com> wrote:

> Hi Martins. You're understanding things correctly, this is a bug in
> output. Will commit a fix soon.
>
> On Wed, Jun 1, 2016 at 3:35 AM, Martin C. <martincs14 at gmail.com> wrote:
>
>> Hi all,
>> I'm new to MESA.
>> I've been playing with binaries. In binary_history_columns.list:
>>       J_orb ! orbital angular momentum
>>       J_spin_1 ! spin angular momentum of first star
>>       J_spin_2 ! spin angular momentum of second star
>>       J_total ! orbital+spin angular momentum
>>
>> It seems that J_total = J_spin_1 + J_spin_2
>> I expected:
>> J_total = J_spin_1 + J_spin_2 + J_orb
>>
>> Am I misunderstanding something?
>>
>> thx,
>>
>> Martin
>>
>> --
>> Martin C.
>>
>>
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>
>
> --
> Pablo Marchant Campos
> M.Sc on Astrophysics, Universidad Católica de Chile
> PhD student, Argelander-Institut für Astronomie
>



-- 
Martin C.
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