  We present a re-organization of the Oh et al. (2017b) (Oh17) wide, co-moving
catalog of 4,555 groups of stars (10,606 individual objects) identified in the
Tycho Gaia Astrometric Survey (TGAS) into new and known co evolving groups of
stars in the Milky Way. We use the BANYAN {\Sigma} kinematic analysis tool to
identify 1,015 individual stars in the Oh17 catalog that yielded a >80%
probability in one of 27 known associations (e.g. the AB Doradus moving group,
Columba, Upper Scorpius) in the vicinity of the Sun. Among the 27 groups
uncovered by Oh17 that had > 10 connected components, we find that 6 are newly
discovered. We use a combination of Tycho, Gaia, 2MASS, WISE, Galex, and ROSAT
photometry as well as Gaia parallaxes to determine that these new groups are
likely older than the Pleiades but younger than ~1 Gyr. Using isochrone fitting
we find that the majority of these new groups have solar type stars and solar
type metallicity. Among the 35 Oh17 groups with 5 - 9 members, we find that 19
also appear new and co-moving, with one group well within 100pc (range of 77 -
90 pc). For known star forming regions, open clusters, and moving groups
identified by Oh17, we find that the majority were broken up into pieces over
several Oh17 groups (e.g. Lower Centaurus Crux members are spread over 26 Oh17
groups) however we found no correlation with positions of the groups on color
magnitude diagrams therefore no substructure of the association correlated with
the Oh17 designated group. We find that across the 27 groups tested by BANYAN
{\Sigma} there were 400 new members to 20 different associations uncovered by
Oh17 that require further vetting.
