The unseen companion of HD114762: a probable brown dwarf

@article{Latham1989TheUC,
  title={The unseen companion of HD114762: a probable brown dwarf},
  author={David W. Latham and Tsevi Mazeh and Robert P. Stefanik and Michel Mayor and Gilbert Burki},
  journal={Nature},
  year={1989},
  volume={339},
  pages={38-40}
}
BROWN dwarfs are substellar objects with too little mass to ignite hydrogen in their cores. Despite considerable effort to detect brown dwarfs astrometrically1–4, photometrically4–9, and spectroscopi-cally10–12, only a few good candidates have been discovered. Here we present spectroscopic evidence for a probable brown-dwarf companion to the solar-type star HD114762. This star undergoes periodic variations in radial velocity which we attribute to orbital motion resulting from the presence of an… 
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Determining the mass of the planetary candidate HD 114762 b using Gaia
  • F. Kiefer
  • Physics, Geology
    Astronomy & Astrophysics
  • 2019
The first planetary candidate discovered by Latham et al. (1989, Nature, 339, 38) with radial velocities around a solar-like star other than the Sun, HD 114762 b, was detected with a minimum mass of
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