eROSITA calibration and performance verification phase: High-mass X-ray binaries in the Magellanic Clouds

The Early Data Release of eROSITA and Mikhail Pavlinsky ART-XC on the SRG mission

Open Access

Fig. 2

SMC mosaic from eROSITA observations around the supernova remnant 1E0102.2–7219, the brightest source near the image centre. Image colours and labels for the HMXB pulsars are as in Fig. 1. HMXBs without known pulse period are indicated by green circles and their entry number from HS16 (see Table 4).

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