  This paper presents multiwavelength observations of a flare-generated type II
radio burst. The kinematics of the shock derived from the type II closely match
a fast EUV wave seen propagating through coronal arcade loops. The EUV wave was
closely associated with an impulsive M1.0 flare without a related coronal mass
ejection, and was triggered at one of the footpoints of the arcade loops in
active region NOAA 12035. It was initially observed in the AIA 335 \AA\ images
with a speed of ~800 km/s and accelerated to ~1490 km/s after passing through
the arcade loops. A fan-spine magnetic topology was revealed at the flare site.
A small, confined filament eruption (~340 km/s) was also observed moving in the
opposite direction to the EUV wave. We suggest that breakout reconnection in
the fan-spine topology triggered the flare and associated EUV wave that
propagated as a fast shock through the arcade loops.
