Sanyukta Agarwal, J. S. Yadav
Published 2022-09-15Version 1
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).
Comments: 4 pages, 4 figures
Scale-invariance of black hole accretion: modeling emission from black hole X-ray binary with relativistic accretion flow simulations
MAXI: all-sky observation from the International Space Station
Constraints on Relativistic Jets in Quiescent Black Hole X-ray Binaries from Broadband Spectral Modeling
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