  Caustic rings of dark matter with $\textit{tricusp}$ cross-section were
predicted to lie in the galactic disk. Their radii increase on cosmological
time scales at a rate of order $1$ kpc/Gyr. When a caustic ring passes through
the orbit of a star, the orbit is strongly perturbed. We find that a star
moving in a nearly circular orbit is first attracted towards the caustic ring,
then moves with and oscillates about the caustic for approximately $1$ Gyr
before returning to its original orbit. As a result, a stellar overdensity
forms around the caustic ring. We predict such overdensities to be of order
$120\%$ near the 2nd caustic ring where the Monoceros Ring is observed and of
order $45$, $30$ and $15\%$ near the 3rd, 4th and 5th caustic rings,
respectively. We show that the associated bulk velocities of the stars near the
caustic rings are less than a few km/s. We also determine the density profile
of interstellar gas near the 5th caustic ring assuming it is in thermal
equilibrium in the gravitational potential of the caustic and of the gas
itself.
