{
  "id": "1701.02871",
  "version": "v1",
  "published": "2017-01-11T07:43:28.000Z",
  "updated": "2017-01-11T07:43:28.000Z",
  "title": "Mass growth in MYSO fed by companion",
  "authors": [
    "Xi Chen",
    "Zhiyuan Ren",
    "Qizhou Zhang",
    "Zhiqiang Shen",
    "Keping Qiu"
  ],
  "comment": "7 figures, 2 tables, accepted to ApJ",
  "categories": [
    "astro-ph.GA"
  ],
  "abstract": "We present a Submillimeter Array (SMA) observation towards the young massive double-core system G350.69-0.49. This system consists of a northeast (NE) diffuse gas Bubble and a southwest (SW) massive young stellar object (MYSO), both clearly seen in the Spitzer images. The SMA observations reveal a gas flow between the NE Bubble and the SW MYSO in a broad velocity range from 5 to 30 km/s with respect to the system velocity. The gas flow is well confined within the interval between the two objects, and traces a significant mass transfer from the NE gas Bubble to the SW massive core. The transfer flow can supply the material accreted onto the SW MYSO at a rate of $4.2\\times10^{-4} year^{-1}$. The whole system therefore suggests a mode for the mass growth in MYSO from a gas transfer flow launched from its companion gas clump, despite that the driving mechanism of the transfer flow is not yet fully determined from the current data.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2017-01-11T07:43:28.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "mass growth",
      "sw myso",
      "gas flow",
      "young massive double-core system g350",
      "massive young stellar object"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}