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Study of the q diagram in GX 339-4

High Energy Astrophysical Phenomena 2022-09-16 v1
Authors: Sanyukta Agarwal , J. S. Yadav
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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).

Keywords

black hole x-ray binary gx 339-4 hardness intensity diagram q diagram x-ray outbursts maxi telescope

Cite

@article{arxiv.2209.07166,
  title  = {Study of the q diagram in GX 339-4},
  author = {Sanyukta Agarwal and J. S. Yadav},
  journal= {arXiv preprint arXiv:2209.07166},
  year   = {2022}
}

Comments

4 pages, 4 figures

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