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Fig. 2.

image

Hardness ratio diagrams for sources detected in the four new XMM-Newton observations of the northern disc of M 31. Only sources with hardness ratio errors EHRi <  0.3 are shown. Different symbols are used for different source classes: red diamonds for foreground stars, orange squares for SNRs, cyan triangles for SSSs, light-blue crosses for X-ray binaries, and dark-blue Xs for background sources. Hard sources, which either can be AGNs or X-ray binaries, are marked with purple circles. Small symbols indicate candidates for each class, confirmed classifications are marked with large symbols. Black dots are used for unclassified sources. In HR2–HR3 diagram lines indicate the predicted position for sources with a power-law spectrum (dash-dotted lines) for Γ = 1 (black), 2 (red), 3 (blue) and a disc black-body spectrum (dashed-dot-dotted lines) for kT = 0.5 keV (black), 1.0 keV (light blue), 2.0 keV (green) for different absorbing foreground NH (thin dotted for 1020 cm−2, dashed for 1021 cm−2, and thick solid for 5 × 1021 cm−2).

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