PARS: Paint the Atmospheres of Rotating Stars

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Ada Coda
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PARS: Paint the Atmospheres of Rotating Stars

Post by Ada Coda » Fri Jul 31, 2020 6:49 pm

PARS: Paint the Atmospheres of Rotating Stars

Abstract: 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.

Credit: Lipatov, Mikhail; Brandt, Timothy D.

Site: http://doi.org/10.5281/zenodo.3955185
https://ui.adsabs.harvard.edu/abs/2020arXiv200712779L

Bibcode: 2020ascl.soft07014L

Preferred citation method: https://ui.adsabs.harvard.edu/abs/2020arXiv200712779L

ID: ascl:2007.014
Last edited by Ada Coda on Mon Aug 03, 2020 11:13 pm, edited 1 time in total.
Reason: Updated code entry.

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