We use ASAS V-band and ASAS-SN g-band observations to model the long-period detached eclipsing binary ASASSN-21co. ASAS observations show an eclipse of depth V ~ 0.6 mag in April of 2009. ASAS-SN g-band observations from March of 2021 show an eclipse of similar duration and depth, suggesting an orbital period of 11.9 years. We combine the g-band observations with additional BVRI photometry taken during the eclipse to model the eclipse using PHOEBE. We find that the system is best described by two M giants with a ratio of secondary radius to primary radius of ~0.61. Optical spectra taken during the eclipse are consistent with at least one component of the binary being an M giant, and we find no temporal changes in the spectral features. The eclipse itself is asymmetric, showing an increase in brightness near mid-eclipse, likely due to rotational variability that is too low amplitude to be observed out-of-eclipse.
@article{arxiv.2107.00662,
title = {ASASSN-21co: A detached eclipsing binary with an 11.9 year period},
author = {D. M. Rowan and K. Z. Stanek and Z. Way and C. S. Kochanek and T. Jayasinghe and Todd A. Thompson and H. Barker and F. -J. Hambsch and T. Bohlsen and Stella Kafka and B. J. Shappee and T. W. -S. Holoien and J. L. Prieto},
journal= {arXiv preprint arXiv:2107.00662},
year = {2021}
}