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.
Accepted by AJ. 8 pages, 9 Figures, 5 Tables
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Cited by in corpus (5)
- Spectroscopic orbits of subsystems in multiple stars. VI
- Comparison of Gaia and Hipparcos parallaxes of close visual binary stars and the impact on determinations of their masses
- Spectroscopic Orbits of Subsystems in Multiple Stars. X (Summary)
- Spectroscopic orbits of subsystems in multiple stars. VIII
- Speckle Interferometry of Nearby Multiple Stars: 2007-2019 Positional Measurements and Orbits of Eight Objects