  Sgr A*, the supermassive black hole (SMBH) in our Galaxy, is dormant today,
but it should have gone through multiple gas-accretion episodes in the past
billions of years to grow to its current mass of $4\times10^6\,M_\odot$. Each
episode temporarily ignites the SMBH and turns the Galactic Center into an
active galactic nucleus (AGN). Recently, we showed that the AGN could produce
large amount of hard X-rays that can penetrate the dense interstellar medium in
the Galactic plane. Here we further study the impact of the X-rays on the
molecular chemistry in our Galaxy. We use a chemical reaction network to
simulate the evolution of several molecular species including H2O, CH3OH, and
H2CO, both in the gas phase and on the surface of dust grains. We find that the
X-ray irradiation could significantly enhance the abundances of these species.
The effect is the most significant in those young, high-density molecular
clouds, and could be prominent at a Galactic distance of $8$ kpc or smaller.
The imprint in the chemical abundance is visible even several million years
after the AGN turns off.
