Relative Orbit Orientation in Several Resolved Multiple Systems

@article{Tokovinin2017RelativeOO,
  title={Relative Orbit Orientation in Several Resolved Multiple Systems},
  author={Andrei Tokovinin and David W. Latham},
  journal={The Astrophysical Journal},
  year={2017},
  volume={838},
  pages={54}
}
This work extends the still modest number of multiple stars with known relative orbit orientation. Accurate astrometry and radial velocities are used jointly to compute or update outer and inner orbits in three nearby triple systems HIP 101955 (orbital periods 38.68 and 2.51 years), HIP 103987 (19.20 and 1.035 years), HIP 111805 (30.13 and 1.50 years) and in one quadruple system HIP 2643 (periods 70.3, 4.85 and 0.276 years), all composed of solar-type stars. The masses are estimated from the… Expand
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