A sample of ionised Fe line-emitting X-ray sources in the inner Galactic disc

Open Access

Fig. 14

Comparison of the mean EW_6.7 and $\frac{I_{6.9}}{I_{6.7}}$ $\frac{I_{6.9}}{I_{6.7}}$ for our hard CV and soft source samples with those of the GCXE and GRXE. The measurement uncertainties represent the 1σ standard deviation. The GCXE and GRXE values are taken from Nobukawa et al. (2016).

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