[mesa-users] helium main sequence binary
Ying Qin
Ying.Qin at unige.ch
Sat Sep 12 06:37:35 EDT 2015
Hi Josiah,
Thank you so much for this reply!
I think I should clarify my aim clearly at first. I want to run mesa with a binary system, A Wolf-Rayet(WR) star and a compact star(NS).
1) WR model is set by using this model: 'zams_z2m2_y98.data’ in inlist1.
Also, I use the WR wind(Detmers et al. A&A, 484,831-839,2008). I add WR wind by changing ‘run_star_extras.f’ from src folder, and put
use_other_wind = .true. and x_ctrl(1) = 1.0 in the inlist1. Sorry about the inlist1 I sent you in last email, I forgot to uncomment these two command lines before sending you(I also test Dutch wind)
2) About the two mass and separation of both stars, I put the following command lines in inlist_project(&binary_controls). The distance between the two stars is 48 hrs(0.2d0).
m1 = 10.0d0 ! donor mass in Msun
m2 = 1.40d0 ! companion mass in Msun
initial_period_in_days = 0.2d0
After all setting above, I again run mesa, and now check the results from binary_history.data.
model_number age binary_separation star_1_mass lg_mstar_dot_1
1 3.1622776601683819E+002 9.6975446700026726E+000 3.9637246692135668E+000 -7.1000524704855197E+000
I know WR star lost mass very fast, these results are not what I expect now.
Why does WR star decrease mass from 3.9637246692135668E+000 ? I think the mass of WR should be decreasing from about 10.0.
Why does binary_separation change from 9.6975446700026726E+000 ? Because I initialize this it with 0.2d0.
For these results, I said there were random, Because they are not reasonable.
Also, I want star1 to evolve with zero age and zero model number, and I change these in inlist1:
set_initial_age = .true.
initial_age = 0 ! in years
set_initial_model_number = .true.
initial_model_number = 0
But from the results, we can clearly find it did not work.
I use mea r7624, and copy binary/work directory. I hope my questions are much clearer. The run_star_extra.f and inlist1 are as follows.
I think I missed something important. I am looking forward your reply to refresh my understanding. Thank you in advance!
With my best regards,
Ying
On 12 Sep 2015, at 06:43, Josiah Schwab <jwschwab at berkeley.edu<mailto:jwschwab at berkeley.edu>> wrote:
Hello Ying,
On 11 September 2015 at 13:50 PDT, Ying Qin wrote:
But from the binary_history.data, I find star 1 started to lose mass
from 2.2 at the beginning(about 300 yrs)
And binary_separation is approximately equal to 20 Rsun.
I ran the inlists you sent and didn't see either of these things.
(Though I didn't understand what "from 2.2" meant.)
The first line of binary_history.data had these entries:
age binary_separation lg_mstar_dot_1
3.1622776601683819E+002 3.2382327687009131E+000 -9.8999999999999986E+001
so the expected separation and no mass loss.
So what I had set in the list did not work.
What version of MESA are you using? All I did was use the inlists you
sent with a fresh binary/work directory from r7624.
And mesa seems to create a random initial parameter.
I don't know what this means.
Josiah
-------------- next part --------------
An HTML attachment was scrubbed...
URL: <https://lists.mesastar.org/pipermail/mesa-users/attachments/20150912/f7320932/attachment.html>
-------------- next part --------------
A non-text attachment was scrubbed...
Name: run_star_extras.f
Type: application/octet-stream
Size: 11995 bytes
Desc: run_star_extras.f
URL: <https://lists.mesastar.org/pipermail/mesa-users/attachments/20150912/f7320932/attachment.obj>
-------------- next part --------------
A non-text attachment was scrubbed...
Name: inlist1
Type: application/octet-stream
Size: 6059 bytes
Desc: inlist1
URL: <https://lists.mesastar.org/pipermail/mesa-users/attachments/20150912/f7320932/attachment-0001.obj>
More information about the Mesa-users
mailing list