{
  "id": "1210.0317",
  "version": "v1",
  "published": "2012-10-01T09:01:34.000Z",
  "updated": "2012-10-01T09:01:34.000Z",
  "title": "Interpreting the simultaneous variability of near-IR continuum and line emission in young stellar objects",
  "authors": [
    "D. Lorenzetti",
    "S. Antoniucci",
    "T. Giannini",
    "A. Di Paola",
    "A. A. Arkharov",
    "V. M. Larionov"
  ],
  "comment": "accepted by Astrophysics and Space Scence",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "We present new near-infrared (IR) spectra (0.80-1.35um) of the pre-Main Sequence source PV Cep taken during a monitoring program of eruptive variables we are conducting since some years. Simultaneous photometric and spectroscopic observations are systematically carried out during outburst and quiescence periods. By correlating extinction-free parameters, such as HI recombination lines and underlying continuum, it is possible to infer on the mechanism(s) responsible for their origin. Accretion and mass loss processes have a dominant role in determining the PV Cep irregular variability of both continuum and line emission. The potentialities of the observational modality are also discussed.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2012-10-01T09:01:34.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "young stellar objects",
      "line emission",
      "near-ir continuum",
      "simultaneous variability",
      "pre-main sequence source pv cep"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1007/s10509-012-1266-4",
      "journal": "Astrophysics and Space Science",
      "year": 2013,
      "month": "Feb",
      "volume": 343,
      "number": 2,
      "pages": 535
    },
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1188783,
      "adsabs": "2013Ap&SS.343..535L"
    }
  }
}