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Calculate [Fe/H] for main sequence stars from either J-H vs. H-K relationship (see Leggett+ 1992 and Fig. 12 of Terrien+ 2015 [http://adsabs.harvard.edu/abs/2015ApJS..220...16T]) or g-K vs. J-K (see H…
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I've been doing some runs where I've changed the critical mass ratio at which unstable mass transfer is initiated for naked and evolved naked helium stars (kstar=7,8,9). The runs have been failing par…
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Hi,
I am trying to load some simulation output files from gadget stored in .hdf5 format.
When I run `h5ls -r `, it shows all the fields.
```
h5ls -r snap_m25n256_151.hdf5
/ …
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reported by: @CloudyLex
In both c13_branch and the trunk the following sim aborts before the first zone:
```
########### shape of considered galaxy
table AGN T=1.5e5 k, a(ox)=-1.4, a(uv)=-0.5, a(x)…
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Hi John,
I am working with Miao Li (CCA) to use Pyxsim to generate mock X-ray spectra of the simulated CGM. Since we just started, we would like some help with a few basic uses of Pyxism.
1) Jus…
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Initial Conditions
=============
PRIMARY MASS = 1.0208328796081652
SECONDARY MASS = 0.7022364956055686
P0 = 4.881682292837919,
Parameters:
==========
Pdisk = 1.4311397660850234
convective …
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Hi,
I am getting the following traceback when running `../amuse.sh make_a_star_cluster.py -M 1e4 -type ascii`
`Traceback (most recent call last):
File "make_a_star_cluster.py", line 337, in
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Systematics tests on clusters have shown a bias in both MIST and Bayestar models to systematically underestimate distances to stars in clusters at lower masses. This effect is driven by the prior: all…
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The referee writes
> Massarotti et al. are not the only ones who report a low metallicity for Aldebaran, Liu et al. 2017 report [Fe/H]=-0.27. Sharma et al. (2016) claim -0.16. The choice of values…