  We construct rotating hybrid axion-miniboson stars (RHABSs), which are
asymptotically flat, stationary, axially symmetric solutions of
(3+1)-dimensional Einstein-Klein-Gordon theory. RHABSs consist of a axion field
(ground state) and a free complex scalar field (first excited state). The
solutions of the RHABSs have two types of nodes, including $^1S^2S$ state and
$^1S^2P$ state. For different axion decay constants $f_a$, we present the mass
$M$ of RHABSs as a function of the synchronized frequency $\omega$, as well as
the nonsynchronized frequency $\omega_2$, and explore the mass $M$ versus the
angular momentum $J$ for the synchronized frequency $\omega$ and the
nonsynchronized frequency $\omega_2$ respectively. Furthermore, we study the
effect of axion decay constant $f_a$ and scalar mass $\mu_2$ on the existence
domain of the synchronized frequency $\omega$.
