{
  "id": "1505.03691",
  "version": "v1",
  "published": "2015-05-14T11:38:35.000Z",
  "updated": "2015-05-14T11:38:35.000Z",
  "title": "Investigating 2MASS J06593158-0405277: a FUor burst in a triple system?",
  "authors": [
    "Alessio Caratti o Garatti",
    "Rebeca Garcia Lopez",
    "Tom P. Ray",
    "Jochen Eisloeffel",
    "Bringfried Stecklum",
    "Aleks Scholz",
    "Stefan Kraus",
    "Gerd Weigelt",
    "Alexander Kreplin",
    "Victor Shenavrin"
  ],
  "comment": "Accepted for publication in the Astrophysical Journal Letters",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "FUor outbursts in young stellar objects (YSOs) are the most dramatic events among episodic accretion phenomena. The origin of these bursts is not clear: disk instabilities and/or disk perturbations by an external body being the most viable hypotheses. Here, we report our VLT/SINFONI high angular resolution AO-assisted observations of 2MASS J06593158-0405277, which is undergoing a recently discovered FUor outburst. Our observations reveal the presence of an extended disc-like structure around the FUor, a very low-mass companion (2MASS J06593158-0405277B) at ~100 au in projection, and, possibly, a third closer companion at ~11 au. These sources appear to be young, displaying accretion signatures. Assuming the components are physically linked, 2MASS J06593158-0405277 would then be one of the very few triple systems observed in FUors.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2015-05-14T11:38:35.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "triple system",
      "fuor burst",
      "investigating 2mass",
      "fuor outburst",
      "high angular resolution ao-assisted observations"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}