{
  "id": "1206.2819",
  "version": "v1",
  "published": "2012-06-13T14:29:07.000Z",
  "updated": "2012-06-13T14:29:07.000Z",
  "title": "Initial parameters of neutron stars",
  "authors": [
    "S. B. Popov",
    "R. Turolla"
  ],
  "comment": "4 pages, contribution to the ERPM conferences, Zielona Gora, April 2012",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "A subpopulation of neutron stars (NSs), known as central compact objects (CCOs) in supernova remnants, are suspected to be low-field objects basing on $P$-$\\dot P$ measurements for three of them. The birth rate of low-field NSs is probably comparable with the birth rate of normal radio pulsars. However, among compact objects in High-Mass X-ray Binaries (HMXBs) we do not see robust candidates for low-field NSs. We propose that this contradiction can be solved if magnetic fields of CCOs was buried due to strong fall-back, and then the field emerges on the time scale $10^4$-$10^5$ yrs.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2012-06-13T14:29:07.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "neutron stars",
      "initial parameters",
      "low-field nss",
      "birth rate",
      "central compact objects"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1118137,
      "adsabs": "2012ASPC..466..191P"
    }
  }
}