{
  "id": "2210.00890",
  "version": "v1",
  "published": "2022-09-30T14:58:30.000Z",
  "updated": "2022-09-30T14:58:30.000Z",
  "title": "Evolutionary status of selected post-AGB stars based on Gaia DR3 data",
  "authors": [
    "M. Parthasarathy",
    "Marina. Kounkel",
    "Keivan G. Stassun"
  ],
  "comment": "1 Figure, 2 Tables, To be submitted",
  "categories": [
    "astro-ph.SR",
    "astro-ph.GA"
  ],
  "abstract": "The evolutionary status of 24 post-AGB stars is presented based on Gaia DR3 data. All 24 stars have parallaxes accurate to better than 3 X sigma and have RUWE values less than 1.4. Based on the Gaia DR3 distances the absolute luminosities are derived. For 14 of the stars, the luminosities confirm their post-AGB evolutionary stage. However, V1027 Cyg, which was previously classified as a post-AGB star, is found to have a higher luminosity; thus it may be an evolved, massive, pulsating semi-regular variable star of type G7Ia. For 9 of the stars, the luminosities are lower than 1000 L (sun), indicating that some are post-RGB stars and some are post-HB stars.This paper was completed more than four months ago but there was delay in getting it published.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2022-09-30T14:58:30.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "gaia dr3 data",
      "selected post-agb stars",
      "evolutionary status",
      "luminosity",
      "post-agb evolutionary stage"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}