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

Abstract

We measured the proper motion of a $\gamma$-ray radio-quiet pulsar J0633+0632 using Chandra observations performed in 2009 and 2017. The measured proper motion is $53\pm 15$~mas~yr${}^{-1}$. We found that the proper motion direction does not follow the extension of the J0633+0632 pulsar wind nebula. The J0633+0632 pulsar wind nebula therefore can be a jet-like feature or a misaligned outflow. We also discuss a possible birth cite of the pulsar.

arXiv comment4 pages, 2 figures and 2 tables

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Cited by in corpus (2)

• XMM-Newton observations of a gamma-ray pulsar J0633+0632: pulsations, cooling and large-scale emission
• The environment of TeV halo progenitors