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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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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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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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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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Currently, when running grids, there are several files created, which aren't needed.
E.g. when running single stars, we still create the binary inlists and copy the binary source code. There are mo…
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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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**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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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…
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I'm getting a steep drop in the DCO count between metallicities 0.0215 and 0.0220, and 5-150 M_sol mass range. From 0.0220, the decline suddenly becomes gradual. The slope changes abruptly at 0.0220 (…