  Streams of gas and dust in the inner parsec of the Galactic center form a
distinct feature known as the Minispiral, which has been studied in radio
waveband as well as in the infrared wavebands. A large fraction of the
Minispiral gas is ionized by radiation of OB stars present in the Nuclear Star
Cluster (NSC). Based on the inferred mass in the innermost parsec ($\sim 10^6$
solar masses), over $\sim 10^3$ -- $10^4$ neutron stars should move in the
sphere of gravitational influence of the SMBH. We estimate that a fraction of
them propagate through the denser, ionized medium concentrated mainly along the
three arms of the Minispiral. Based on the properties of the gaseous medium, we
discuss different interaction regimes of magnetised neutron stars passing
through this region. Moreover, we sketch expected observational effects of
these regimes. The simulation results may be applied to other galactic nuclei
hosting NSC, where the expected distribution of the interaction regimes is
different across different galaxy types.
