Spectroscopic orbits of subsystems in multiple stars. V
Solar and Stellar Astrophysics
2019-02-13 v1
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.
Keywords
Cite
@article{arxiv.1901.03655,
title = {Spectroscopic orbits of subsystems in multiple stars. V},
author = {Andrei Tokovinin},
journal= {arXiv preprint arXiv:1901.03655},
year = {2019}
}
Comments
Accepted by AJ. 8 pages, 9 Figures, 5 Tables