Spectroscopic orbits of subsystems in multiple stars. V
arXiv:1901.03655 · doi:10.3847/1538-3881/aafe00
Abstract
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.
arXiv commentAccepted by AJ. 8 pages, 9 Figures, 5 Tables
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