  The local measurement of $H_0$ is in tension with the prediction of
$\Lambda$CDM model based on the Planck data. This tension may imply that dark
energy is strengthened in the late-time Universe. We employ the latest
cosmological observations on CMB, BAO, LSS, SNe, $H(z)$ and $H_0$ to constrain
several interacting dark energy models. Our results show no significant
indications for the interaction between dark energy and dark matter. The $H_0$
tension can be moderately alleviated, but not totally released.
