The family of V1311 Ori: a young sextuple system or a mini-cluster?
  A compact bound group of four active M-type dwarfs containing V1311 Ori is
identified in the Gaia catalog of nearby stars. Located at a distance of 39 pc,
it is likely related to the beta Pictoris and 32 Ori moving groups by
kinematics, isochronal age, and other indicators of youth (Halpha emission,
presence of lithium, and fast rotation). The brightest star A is a known close
binary, for which a preliminary 80-yr visual-spectroscopic orbit is determined.
Star B is resolved here into a 0.08" pair, and the faintest stars C and D are
probably single. Considering the non-hierarchical configuration with projected
separations of ~10 kau, this could be either a young sextuple system or a bound
but dynamically unstable mini-cluster (trapezium) that avoided disruption so
far. This pre-main-sequence system bridges the gap between moving groups and
wide hierarchies.
