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**Describe the bug**
When running a binary star with the SeBa code via AMUSE, the order of the stars (primary or secondary) that is printed in the output file "starev.data" changes depending on the m…
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In the initial_eccentricity_flow_chart, both H-rich and He-rich stars in RLO are being directed to step_HMS_HMS_RLO. However, this step does not actually handle the He-rich stars, it just fails them b…
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There are multiple versions in Zserio like binary encoding version, JSON encoding version, extension version, etc...
It would be good to have badges for them to allow users a quick compatiblity che…
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Investigating the frequency of planets around binary stars was one of Kepler’s prime mission goals, as binary stars and multi-star systems are common. Although some planets have been found to orbit bi…
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**Describe the bug**
The outcomes of stars that spend some time as HeMS stars is showing some convergence issues. I find that the He and CO core masses vary by a lot (in some cases by a factor of ~…
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Binary stars in Noctis IV can be pretty exciting. It'd be nice if they're properly supported, i.e. if the "planet class" 11 ("Companion star - not a planet.") shows as a proper star in space as well.
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I encountered a `KeyError` when attempting to calculate magnitudes for **binary stars** using the isochrones package. The error occurs specifically when accessing the key `'J'` in the `props_A` or `pr…
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Binaries with the parameters ('stripped_He_Central_He_depleted', 'H-rich_Core_H_burning', 'RLO1', 'oRLO1') are failing because they are not handled in the flow. An example of one such binary:
```
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This program below is an attempt to implement the one here : http://www.glowscript.org/#/user/GlowScriptDemos/folder/Examples/program/BinaryStar-VPython/edit
but it doesnt work.. This was on Chrome be…
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Hi I'm a student working with @stephtdouglas measuring periods for binaries. For stars of short periods, the original rejection sampling (without MCMC) is resulting in short eccentricities which is wh…