Chemodynamics of newly identified giants with globular cluster like
  abundance patterns in the bulge, disk, and halo of the Milky Way
  The latest edition of the APOGEE-2/DR14 survey catalogue and the first
\texttt{Payne} data release of APOGEE abundance determinations by Ting et al.
are examined. We identify 31 previously unremarked metal-poor giant stars with
anomalously high levels of nitrogen in the chemical space defined by [Fe/H] and
[N/Fe]. The APOGEE chemical abundance patterns of such objects revealed that
these are chemically distinct from the Milky Way (MW) in most chemical
elements. We have found all these objects have a [N/Fe]$>+0.5$, and are thus
identified here as nitrogen-rich stars. An orbital analysis of these objects
revealed that a handful of them shares the orbital properties of the bar/bulge,
and possibly linked to tidal debris of surviving globular clusters trapped into
the bar component. 3 of the 31 stars are actually halo interlopers into the
bulge area, which suggests that halo contamination is not insignificant when
studying N-rich stars found in the inner Galaxy, whereas the rest of the N-rich
stars share orbital properties with the halo population. Most of the newly
identified population exhibit chemistry similar to the so-called
\textit{second-generation} globular cluster stars (enriched in aluminum,
[Al/Fe]$>+0.5$), whereas a handful of them exhibit lower abundances of
aluminum, [Al/Fe]$<+0.5$, which are thought to be chemically associated with
the \textit{first-generation} of stars, as seen in globular clusters, or
compatible with origin from a tidally disrupted dwarf galaxy.
