{
  "id": "2209.06012",
  "version": "v1",
  "published": "2022-09-13T14:06:31.000Z",
  "updated": "2022-09-13T14:06:31.000Z",
  "title": "Wind parameters of the new LBV in NGC1156",
  "authors": [
    "Y. Solovyeva",
    "A. Kostenkov",
    "E. Dedov",
    "A. Vinokurov"
  ],
  "comment": "Submitted to Proceedings of Science. Conference \"The Multifaceted Universe: Theory and Observations - 2022 (MUTO2022)\", 23-27 May 2022, SAO RAS, Nizhny Arkhyz, Russia",
  "categories": [
    "astro-ph.SR",
    "astro-ph.GA"
  ],
  "abstract": "In this work we present the spectrum modeling results for the newly discovered luminous blue variable (LBV) in the NGC 1156 galaxy. Extended atmosphere models were calculated using the non-LTE code CMFGEN. We have obtained the luminosity of the discovered LBV $L\\simeq (1.6\\pm0.2) \\times 10^{5} L_{\\odot}$, effective temperature $T_{\\text{eff}}=7.9\\pm0.4$ kK and mass-loss rate $\\dot{M}f^{-0.5}= (8.2\\pm1.0) \\times 10^{-4} M_{\\odot}\\text{yr}^{-1}$. The hydrogen abundance in the wind is $\\approx20\\,$% for the metallicity $Z=0.5 Z_{\\odot}$ of the host galaxy.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2022-09-13T14:06:31.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "wind parameters",
      "non-lte code cmfgen",
      "mass-loss rate",
      "spectrum modeling results",
      "host galaxy"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}