Rotational variables are stars that vary in brightness due to star spots modulated by rotation. They are probes of stellar magnetism, binarity, and evolution. Phillips et al. (2023) explored distinct populations of ~50,000 high-amplitude rotational variables from the All-Sky Automated Survey for Supernovae (ASAS-SN), examining correlations between stellar rotation, binarity, and activity. Here, we carry out a similar analysis of ~50,000 much lower amplitude Kepler rotational variables. The Kepler population is dominated by slowly rotating, single, main sequence stars, with a striking absence of the rapidly rotating main sequence group in the ASAS-SN sample. The binary fractions of the Kepler rotators are significantly lower than for the ASAS-SN systems and they are significantly less spotted, as expected from their lower amplitudes. The scope of these statistical surveys will dramatically increase in the near future.
@article{arxiv.2506.13919,
title = {Rotational Variables: Kepler Versus ASAS-SN},
author = {Jack Stethem and Christopher S. Kochanek and Anya Phillips and Lyra Cao and Marc Pinsonneault},
journal= {arXiv preprint arXiv:2506.13919},
year = {2025}
}