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We measured the proper motion of a $\gamma$-ray radio-quiet pulsar J0633+0632using Chandra observations performed in 2009 and 2017. The measured propermotion is $53\pm15$~mas~yr$^{-1}$. We found that the proper motion directiondoes not follow the extension of the J0633+0632 pulsar wind nebula. TheJ0633+0632 pulsar wind nebula therefore can be a jet-like feature or amisaligned outflow. We also discuss a possible birth cite of the pulsar.

Chandra measurements of the proper motion of the $\gamma$-ray pulsar J0633+0632