Flux-resolved X-ray spectroscopy of GX 17+2 yields a nearly constant accretion efficiency near 0.2, with the normal branch driven by inner-disk and coronal geometry while the flaring branch is driven by an increased accretion rate.
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Spectral evolution of GX 17+2 using AstroSat and NICER observations
Flux-resolved X-ray spectroscopy of GX 17+2 yields a nearly constant accretion efficiency near 0.2, with the normal branch driven by inner-disk and coronal geometry while the flaring branch is driven by an increased accretion rate.