http://arxiv.org/abs/1901.03655
Spectroscopic orbits are determined for inner subsystems in nine stellar hierachies (HIP 2863, 4974, 8353, 28796, 35261, 92929, 115272, 115552, and 117596). Their periods range from 2.5 to 312 days. For each system, estimates of masses, orbital inclination and other parameters are given.
A. Tokovinin
Mon, 14 Jan 19
18/43
Comments: Accepted by AJ. 8 pages, 9 Figures, 5 Tables
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