  Kink oscillations, which are frequently observed in coronal loops and
prominences, are often accompanied by extreme-ultraviolet (EUV) waves. However,
much more needs to be explored regarding the causal relationships between kink
oscillations and EUV waves. In this article, we report the simultaneous
detection of kink oscillations and EUV waves that are both associated with an
X2.1 flare on 2023 March 03 (SOL2023-03-03T17:39). The kink oscillations, which
are almost perpendicular to the axes of loop-like structures, are observed in
three coronal loops and one prominence. One short loop shows in-phase
oscillation within the same period of 5.2 minutes at three positions. This
oscillation could be triggered by the pushing of an expanding loop and
interpreted as the standing kink wave. Time lags are found between the kink
oscillations of the short loop and two long loops, suggesting that the kink
wave travels in different loops. The kink oscillations of one long loop and the
prominence are possibly driven by the disturbance of the CME, and that of
another long loop might be attributed to the interaction of the EUV wave. The
onset time of the kink oscillation of the short loop is nearly same as the
beginning of an EUV wave. This fact demonstrates that they are almost
simultaneous. The EUV wave is most likely excited by the expanding loop
structure and shows two components. The leading component is a fast coronal
wave, and the trailing one could be due to the stretching magnetic field lines.
