论文标题

$γ$ -Ray pulsar J0633+0632的正确运动的Chandra测量值

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

论文作者

Danilenko, Andrey, Karpova, Anna, Shibanov, Yury

论文摘要

我们使用Chandra观测值在2009年和2017年进行的Chandra观测值测量了$γ$ -ROAR ROAVIT-QUIET PULSAR J0633+0632。测量的适当运动为$ 53 \ pm15 $ 〜mas〜mas〜yr $^yr $^{ - 1} $。我们发现,正确的运动方向不会遵循J0633+0632脉冲星云的延伸。因此,J0633+0632 Pulsar风星云可以是类似喷射的特征或未对准的流出。我们还讨论了可能出生的脉冲星。

We measured the proper motion of a $γ$-ray radio-quiet pulsar J0633+0632 using Chandra observations performed in 2009 and 2017. The measured proper motion is $53\pm15$~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.

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