{
  "id": "1812.10767",
  "version": "v1",
  "published": "2018-12-27T16:50:47.000Z",
  "updated": "2018-12-27T16:50:47.000Z",
  "title": "Inference on Disk-Jet Connection of MAXI~J1836-194: Analysis with the TCAF Solution",
  "authors": [
    "Arghajit Jana",
    "Dipak Debnath",
    "Sandip K. Chakrabarti",
    "Debjit Chatterjee"
  ],
  "comment": "12 pages, 5 figures, 2 tables",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "Galactic transient black hole candidate (BHC) MAXI~J1836-194 was discovered on 2011 Aug 30, by MAXI/GSC and Swift/BAT. The source activity during this outburst was continued for $\\sim 3$ months before entering into the quiescent state. It again became active in March 2012 and continued for another $\\sim 2$ months. In this paper, $3-25$ $keV$ RXTE/PCA spectra of 2011 outburst and $0.5-10.0$ $keV$ Swift/XRT data during its 2012 outburst are analyzed with the two-component advective flow (TCAF) model based fits file in XSPEC. We calculate the X-ray contributions coming from jets/outflow using a newly developed method based on the deviation of the TCAF model normalization. We also studied the correlation between observed radio and estimated jet X-ray fluxes. The correlation indices ($b$) are found to be $1.79$, and $0.61$, when the $7.45$~GHz VLA radio flux is correlated with the total X-ray and the jet X-ray fluxes in $3-25$ keV range respectively. It has been found that the jet contributes in X-rays up to a maximum of 86\\% during its 2011 outburst. This makes the BHC MAXI~J1836-194 to be strongly jet dominated during the initial rising phase.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2018-12-27T16:50:47.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "tcaf solution",
      "disk-jet connection",
      "galactic transient black hole candidate",
      "ghz vla radio flux",
      "estimated jet x-ray fluxes"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 12,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}