Astrometry and Precise Radial Velocities Yield a Complete Orbital Solution for the Nearby Eccentric Brown Dwarf LHS 1610 b

We characterize the LHS 1610 system, a nearby (d=9.7 pc) M5 dwarf hosting a brown dwarf in a 10.6 day, eccentric (e \sim 0.37) orbit. A joint fit of the available Gaia two-body solution, discovery radial velocities (RVs) from TRES, and new RVs obtained with the Habitable-zone Planet Finder, yields... Show more