{
  "id": "1912.12639",
  "version": "v1",
  "published": "2019-12-29T11:48:50.000Z",
  "updated": "2019-12-29T11:48:50.000Z",
  "title": "Third components with elliptical orbits in the eclipsing binaries: EQ Tau, IR Cas, IV Cas, RY Aqr & RZ Com",
  "authors": [
    "D. E. Tvardovskyi"
  ],
  "comment": "6 pages, 6 figures, submitted to Annaly Astronomii Nowej",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "This research is our forth article related to the topic of cyclic O-C changes, third components as the physical process that cause these changes and elliptical orbits of the third components. Here five more eclipsing binary stars were investigated: EQ Tau, IR Cas, IV Cas, RY Aqr and RZ Com. All of them have cyclic O-C curve with superposition of parabolic trend. We computed the mass transfer rate, minima possible mass of the third component and their errors for each of the researched stars.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2019-12-29T11:48:50.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "third component",
      "ry aqr",
      "eq tau",
      "ir cas",
      "eclipsing binary"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 6,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}