  Observations of tidal disruption events (TDEs) show signs of Nitrogen
enrichment reminiscent of other astrophysical sources such as active galactic
nuclei (AGN) and star-forming galaxies. Given that TDEs probe the gas from a
single star, it is possible to test if the observed enrichment is consistent
with expectations from the CNO cycle by looking at the observed Nitrogen/Carbon
(N/C) abundance ratios. Given that $\approx 20\%$ of solar mass stars (and an
even larger fraction of more massive stars) live in close binaries, it is
worthwhile to also consider what TDEs from stars influenced by binary evolution
would look like. We show here that TDEs from stars stripped of their
Hydrogen-rich (and Nitrogen-poor) envelopes through previous binary-induced
mass loss can produce much higher observable N/C enhancements than even TDEs
from massive stars. Additionally, we predict that the time-dependence of the
N/C abundance ratio in the mass fallback rate of stripped stars will follow the
inverse behavior of main-sequence stars, enabling a more accurate
characterization of the disrupted star.
