Fig. 2
Correlation of the residual mass accretion rate and the residual X-ray luminosity. Left: residual mass accretion rate as a function of residual X-ray luminosity. The regression line was obtained with the Bayesian LINMIX_ERR method, and the shaded region shows its 1σ scatter. The cross indicates the typical uncertainties. There is a weak anticorrelation. Right: residual mass accretion rate as a function of the residual soft band (0.5–2.0 keV) X-ray luminosity. The anticorrelation is stronger and more significant.
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