{
  "id": "2001.09871",
  "version": "v1",
  "published": "2020-01-27T15:48:46.000Z",
  "updated": "2020-01-27T15:48:46.000Z",
  "title": "Chandra measurements of the proper motion of the $γ$-ray pulsar J0633+0632",
  "authors": [
    "Andrey Danilenko",
    "Anna Karpova",
    "Yury Shibanov"
  ],
  "comment": "4 pages, 2 figures and 2 tables",
  "journal": "2019, JPhCS, 022017, JPhCS1400",
  "doi": "10.1088/1742-6596/1400/2/022017",
  "categories": [
    "astro-ph.HE",
    "astro-ph.SR"
  ],
  "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 $53\\pm15$~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.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2020-01-27T15:48:46.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "ray pulsar",
      "chandra measurements",
      "pulsar wind nebula",
      "ray radio-quiet pulsar",
      "proper motion direction"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "publisher": "IOP"
    },
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}