{
  "id": "2209.07166",
  "version": "v1",
  "published": "2022-09-15T09:36:38.000Z",
  "updated": "2022-09-15T09:36:38.000Z",
  "title": "Study of the q diagram in GX 339-4",
  "authors": [
    "Sanyukta Agarwal",
    "J. S. Yadav"
  ],
  "comment": "4 pages, 4 figures",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "Black hole X-ray binary (BHXB) GX 339-4 produces the most frequent X-ray outbursts (every 2-4 years) among known X-ray binary sources in our galaxy. Here we present the study of the evolution of GX 339-4 over the years of observations using the Hardness Intensity Diagram (HID), i.e., the q diagram. We present an analysis of two outbursts of the source observed by the Monitor of All-sky X-ray Image (MAXI) telescope aboard the International Space Station (ISS).",
  "revisions": [
    {
      "version": "v1",
      "updated": "2022-09-15T09:36:38.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "black hole x-ray binary",
      "international space station",
      "hardness intensity diagram",
      "x-ray binary sources",
      "frequent x-ray outbursts"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}