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- W2805651612 abstract "Spectroscopic orbits are computed for inner pairs in six nearby hierarchical multiple systems (HIP 35733, 95106/95110, 105441, 105585/105569, 105947, and 109951). Radial velocities and resolved measurements, when available, are used to derive combined sets of outer orbital elements for three systems. Each multiple system is discussed individually. Additionally, HIP 115087 is a simple 7.9-day single-lined binary. Although the minimum companion mass is substellar (in the brown dwarf desert regime), it appears to be a 0.2 solar-mass star in a low-inclination orbit." @default.
- W2805651612 created "2018-06-13" @default.
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- W2805651612 date "2018-07-12" @default.
- W2805651612 modified "2023-09-26" @default.
- W2805651612 title "Spectroscopic Orbits of Subsystems in Multiple Stars. III." @default.
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- W2805651612 doi "https://doi.org/10.3847/1538-3881/aacb78" @default.
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