{
  "id": "1802.05850",
  "version": "v1",
  "published": "2018-02-16T07:15:12.000Z",
  "updated": "2018-02-16T07:15:12.000Z",
  "title": "Study of Magnetized accretion flow with cooling processes",
  "authors": [
    "Kuldeep Singh",
    "Indranil Chattopadhyay"
  ],
  "comment": "8 pages, 6 figures, published in a special issue of JApA",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "We have studied shock in magnetized accretion flow/funnel flow in case of neutron star with bremsstrahlung cooling and cyclotron cooling. All accretion solutions terminate with a shock close to the neutron star surface, but at some region of the parameter space, it also harbours a second shock away from the star surface. We have found that cyclotron cooling is necessary for correct accretion solutions which match the surface boundary conditions.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2018-02-16T07:15:12.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "cooling processes",
      "magnetized accretion flow/funnel flow",
      "accretion solutions terminate",
      "correct accretion solutions",
      "neutron star surface"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 8,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}