{
  "id": "0909.3062",
  "version": "v1",
  "published": "2009-09-16T17:16:56.000Z",
  "updated": "2009-09-16T17:16:56.000Z",
  "title": "Orbital parameters of binary radio pulsars in globular clusters and stellar interactions",
  "authors": [
    "Manjari Bagchi",
    "Alak Ray"
  ],
  "comment": "Published in the Low-Frequency Radio Universe ASP Conference Series, Vol. 407, proceedings of the conference held 8-12 December 2008, at National Centre for Radio Astrophysics (NCRA), TIFR, Pune, India. Edited by D. J. Saikia, D. A. Green, Y. Gupta, and T. Venturi. San Francisco: Astronomical Society of the Pacific",
  "journal": "ASPC 407 (2009) 353",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "The observed distribution of globular cluster binary radio pulsars in the eccentricity versus orbital period plane can be explained as a result of binary-single star interactions. Our numerical and analytical study hints that the highest eccentricity binaries in clusters are likely to be from exchange and/or merger of a single star with a binary component, while the intermediate eccentricity systems are probably results of fly-by interactions.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2009-09-16T17:16:56.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "orbital parameters",
      "stellar interactions",
      "globular cluster binary radio pulsars",
      "orbital period plane",
      "intermediate eccentricity systems"
    ],
    "tags": [
      "conference paper",
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 831458,
      "adsabs": "2009ASPC..407..353B"
    }
  }
}