{
  "id": "2007.12383",
  "version": "v1",
  "published": "2020-07-24T07:15:35.000Z",
  "updated": "2020-07-24T07:15:35.000Z",
  "title": "Absolute physical parameters of three poorly studied detached eclipsing binaries",
  "authors": [
    "D. -Y. Yang",
    "L. -F. Li",
    "Q. -W. Han"
  ],
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "The photometric and spectroscopic data for three double-lined detached eclipsing binaries were collected from the photometric and spectral surveys. The light and radial velocity curves of each binary system were simultaneously analyzed by using Wilson-Devinney (WD) code, and the absolute physical and orbital parameters of these binaries were derived. The masses of both components of ASASSN-V J063123.82+192341.9 were found to be $M_1 = 1.088 \\pm 0.016$ and $M_2 = 0.883 \\pm 0.016\\ M_{\\odot}$; and those of ASAS J011416+0426.4 were determined to be $M_1 = 0.934 \\pm 0.046$ and $M_2 = 0.754 \\pm 0.043 M_{\\odot}$; those of MW Aur were derived to be $M_1 = 2.052 \\pm 0.196$ and $M_2 = 1.939 \\pm 0.193\\ M_{\\odot}$. At last, the evolutionary status of these detached binaries was discussed based on their absolute parameters and the theoretical stellar models. Keywords: Stars: binaries: eclipsing $-$ stars: fundamental parameters$-$ stars: evolution $-$ stars: individual: ASASSN-V J063123.82+192341.9, ASAS J011416+0426.4 and MW Aur",
  "revisions": [
    {
      "version": "v1",
      "updated": "2020-07-24T07:15:35.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "detached eclipsing binaries",
      "absolute physical parameters",
      "mw aur",
      "radial velocity curves",
      "binary system"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}