{
  "id": "2003.09511",
  "version": "v1",
  "published": "2020-03-20T21:53:21.000Z",
  "updated": "2020-03-20T21:53:21.000Z",
  "title": "Accretion in low-mass members of the Orion Nebula Cluster with young transition disks",
  "authors": [
    "R. M. G. de Albuquerque",
    "J. F. Gameiro",
    "S. H. P. Alencar",
    "J. J. G. Lima",
    "C. Sauty",
    "C. Melo"
  ],
  "comment": "12 pages, 6 figures (17 pages, 11 figures if appendix included). Accepted by Astronomy and Astrophysics on 24/02/2020",
  "categories": [
    "astro-ph.SR",
    "astro-ph.EP",
    "astro-ph.GA"
  ],
  "abstract": "Although the Orion Nebula Cluster is one of the most studied clusters in the solar neighborhood, the evolution of the very low-mass members ($M_* < 0.25 \\, M_\\odot$) has not been fully addressed due to their faintness. Our goal is to verify if some young and very low-mass objects in the Orion Nebula Cluster show evidence of ongoing accretion using broadband VLT/X-Shooter spectra. For each target, we determined the corresponding stellar parameters, veiling, observed Balmer jump, and accretion rates. Additionally, we searched for the existence of circumstellar disks through available on-line photometry. We detected accretion activity in three young stellar objects in the Orion Nebula Cluster, two of them being in the very low-mass range. We also detected the presence of young transition disks with ages between 1 and 3.5 Myr.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2020-03-20T21:53:21.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "orion nebula cluster",
      "young transition disks",
      "low-mass members",
      "young stellar objects",
      "broadband vlt/x-shooter spectra"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 12,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}