2021•Research Notes of the AASOpen access
ASASSN-21co: A Detached Eclipsing Binary with an 11.9 yr Period
D. M. Rowan, K. Z. Stanek, Z. Way, C. S. Kochanek, T. Jayasinghe, Todd A. Thompson, Hamish Barker, Franz-Josef Hambsch, T. Bohlsen, S. Kafka, B. J. Shappee, T. W. S. Holoien, J. L. Prieto
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Abstract
Abstract 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 2009 April. ASAS-SN g-band observations from 2021 March show an eclipse of similar duration and depth, suggesting an orbital period of 11.9 yr. 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.