  We investigate the impact of anomalous microwave emission (AME) on the
radio-millimeter spectral energy distribution for three typical interstellar
medium (ISM) conditions surrounding star-forming regions -- cold neutral
medium, warm neutral medium, and photodissociation region -- by comparing the
emissivities of three major contributors: free-free, thermal dust emission, and
AME. In particular, for spinning nanoparticles (i.e., potential carriers of
AME), we consider a known grain destruction mechanism due to a centrifugal
force from spin-up processes caused by collisions between dust grains and
supersonic neutral streams in a magnetized shock (C-shock). We demonstrate
that, if the ISM in a magnetic field is impacted by a C-shock developed by a
supernova explosion in the early phase of massive star-formation ($\lesssim 10$
Myr), AME can be significantly or almost entirely suppressed relative to
free-free and thermal dust continuum emission if the grain tensile strength is
small enough. This study may shed light on explaining the rare observations of
AME from extragalactic star-forming regions preferentially observed from
massive star clusters and suggest a scenario of "the rise and fall of AME" in
accordance with the temporal evolution of star-forming regions.
