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[ascl:2007.014] PARS: Paint the Atmospheres of Rotating Stars

PARS (Paint the Atmospheres of Rotating Stars) quickly computes magnitudes and spectra of rotating stellar models. It uses the star's mass, equatorial radius, rotational speed, luminosity, and inclination as input; the models incorporate Roche mass distribution (where all mass is at the center of the star), solid body rotation, and collinearity of effective gravity and energy flux.

Code site:
https://github.com/mlipatov/paint_atmospheres http://doi.org/10.5281/zenodo.3955185
Described in:
https://ui.adsabs.harvard.edu/abs/2020arXiv200712779L
Bibcode:
2020ascl.soft07014L

Views: 443

ascl:2007.014
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