{
  "id": "1808.09620",
  "version": "v1",
  "published": "2018-08-29T03:28:15.000Z",
  "updated": "2018-08-29T03:28:15.000Z",
  "title": "Turbulent convection and pulsation stability of stars - III. Non-adiabatic oscillations of red giants",
  "authors": [
    "D. R. Xiong",
    "L. Deng",
    "C. Zhang"
  ],
  "comment": "7 pages, 6 figures, published 2018 August 2",
  "journal": "MNRAS, 480, 2698-2703 (2018)",
  "doi": "10.1093/mnras/sty2014",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "We have computed linear non-adiabatic oscillations of luminous red giants using a non-local and anisotropic time-dependent theory of convection. The results show that low-order radial modes can be self-excited. Their excitation is the result of radiation and the coupling between convection and oscillations. Turbulent pressure has important effects on the excitation of oscillations in red variables.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2018-08-29T03:28:15.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "red giants",
      "turbulent convection",
      "pulsation stability",
      "low-order radial modes",
      "anisotropic time-dependent theory"
    ],
    "tags": [
      "journal article"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 7,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}