{
  "id": "2106.05049",
  "version": "v1",
  "published": "2021-06-09T13:02:39.000Z",
  "updated": "2021-06-09T13:02:39.000Z",
  "title": "One is the loneliest number: multiplicity in cool dwarfs",
  "authors": [
    "Carlos Cifuentes",
    "Jose A. Caballero",
    "Sergio Agusti"
  ],
  "comment": "4 pages, 1 table. GitHub repository: https://github.com/ccifuentesr/cif21-multiplicity/",
  "journal": "2021RNAAS...5..129C",
  "doi": "10.3847/2515-5172/ac05ce",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "Stars in multiple systems offer a unique opportunity to learn about stellar formation and evolution. As they settle down into stable configurations, multiple systems occur in a variety of hierarchies and a wide range of separations between the components. We examine 11 known and 11 newly discovered multiple systems including at least one M dwarf with the latest astrometric data from Gaia Early Data Release 3 (EDR3). We find that the individual components of systems at very wide separations are often multiple systems themselves.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2021-06-09T13:02:39.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "cool dwarfs",
      "loneliest number",
      "multiplicity",
      "multiple systems occur",
      "latest astrometric data"
    ],
    "tags": [
      "github project",
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}