[mesa-users] Extended helium envelopes
Bill Paxton
paxton at kitp.ucsb.edu
Thu Oct 24 19:28:16 EDT 2013
Hi Craig,
Send an inlist and a saved model after removing envelope but before it expands.
Then we can try it ourselves to see what might be going on.
Thanks,
Bill
On Oct 24, 2013, at 2:44 PM, Craig Wheeler wrote:
> Hi all,
>
> We are trying to make ad hoc "Wolf-Rayet" models with MESA by stripping
> off the hydrogen envelope by hand from massive star models near the
> end of helium core burning. We are finding that the resulting "stripped
> envelope" models evolve normally for a while, but then are prone to
> having the remaining helium envelope expand to red-giant size,
> 100 R_sun or so. There is no question this can happen in some
> circumstances, for instance stars with a substantial helium abundance
> and a helium-burning shell atop a degenerate carbon/oxygen core, the
> supposed the structure of R Cor Bor stars. I have, however, no
> recollection of this expanding helium envelope phenomenon occurring
> in more massive, non-degenerate cores. The issue seems more acute
> for lower mass cores, a few to 10 solar masses, but may be related to
> opacity bumps, Eddington luminosity and radiation pressure. It also
> seems to be exacerbated by rotation.
>
> Any perspective on this issue would be appreciated.
>
> Thanks,
>
> Craig
>
> --
> J. Craig Wheeler
> Department of Astronomy
> 2515 Speedway, Stop C1400
> Austin, TX 78712-1205
> 512-471-6407
> http://www.as.utexas.edu/~wheel
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> http://www.smashwords.com/books/view/178104
> http://www.amazon.com/The-Krone-Experiment-ebook/dp/B008Y6L3VW
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> http://www.amazon.com/The-Q-Man-1-ebook/dp/B00AFKJYKC
>
>
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