Abstract
HR 4693 is a fifth-magnitude K2 III star whose radial-velocity nature has been the subject of conflicting ideas. It is shown here to be a spectroscopic binary of small amplitude, less than 2 km s-1; the orbit is quite eccentric and has a period of 16 years
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Griffin, R.F. Spectroscopic binaries near the North Galactic Pole paper 19: HR 4693. J Astrophys Astron 12, 39–48 (1991). https://doi.org/10.1007/BF02709771
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DOI: https://doi.org/10.1007/BF02709771