Spectroscopic Orbits of Subsystems in Multiple Stars. V.

Tokovinin, Andrei

Chile

Abstract

Spectroscopic orbits are determined for inner subsystems in nine stellar hierarchies (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.

2019 The Astronomical Journal
Gaia Hipparcos 12