Identification of three cataclysmic variables detected by the ART-XC and eROSITA telescopes on board the SRG during the all-sky X-ray survey

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

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Fig. 5

Zoom into the 4550–4950 Å range of the optical spectrum of SRGA J204547.8+672642. The Bowen blend and H_β are visible, while HeIIλ4686 is not significantly detected.

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