[mesa-users] Pre-MS to Wolf-Rayet Evolution Problem

Matteo Cantiello cantiel at kitp.ucsb.edu
Sun Oct 16 12:19:06 EDT 2016


Dear Irham,
It’s difficult to determine what problem you are experiencing from your description. 
I have a few ideas, but if you want MESA users to help, the best way would be to send diagnostic plots of your models.
Incidentally, examining what’s the internal state of your model (plotting different quantities), could help you find some answers to your own questions and/or learn more about the evolution of stars.

As a side note, the TPAGB phase (thermally pulsating asymptotic giant branch) is not an evolutionary phase expected for a 32 Msun star.

If you are interested in the challenges of evolving rotating, very massive stars, I suggest you first also have a look at the second mesa instrument paper (http://adsabs.harvard.edu/abs/2013ApJS..208....4P <http://adsabs.harvard.edu/abs/2013ApJS..208....4P>, in particular Sec.7).
Cheers,

-M

Matteo Cantiello  |  http://matteocantiello.com/ 
Specialist in Astrophysics  | Kavli Institute for Theoretical Physics
Chief Scientist and Board Member, Authorea  |  https://www.authorea.com/

> On Oct 16, 2016, at 5:05 AM, Irham Taufik <irham.andika at gmail.com> wrote:
> 
> Dear all,
> 
> Currently I use MESA to create evolution model of 32 M_sun star from pre-MS to Wolf-Rayet phase. However, it seems the program only works until TPAGB and cannot reach WR phase. I attached my inlist file in this email. Is there something wrong with my input parameters?
> 
> Best regards,
> Irham
> 
> 
> 
> -- 
> Irham Taufik Andika
> Astronomy Study Program
> Bandung Institute of Technology, Indonesia
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