Abstract
HD 111154 is a member of the Coma Cluster. It is here shown to be a somewhat unequal pair of stars of approximately solar type. They are in an orbit that has a period of just under 27 days and quite a high eccentricity (0.442). Although the minimum masses (1.08 and 1.00M ⊙) are large enough to encourage a search for eclipses, no such events have been detected.
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Griffin, R.F. Spectroscopic binaries near the North Galactic Pole paper 23: HD 111154. J Astrophys Astron 22, 121–130 (2001). https://doi.org/10.1007/BF02933592
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DOI: https://doi.org/10.1007/BF02933592