Spectroscopic radial velocities confirm that the Be primary of V1624 Cyg moves on the 359.26-day circular orbit found by interferometry, with a low-mass compact secondary of about 0.66 solar masses.
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Spectroscopic orbit and variability of the Be star V1624 Cyg = 28 Cyg
Spectroscopic radial velocities confirm that the Be primary of V1624 Cyg moves on the 359.26-day circular orbit found by interferometry, with a low-mass compact secondary of about 0.66 solar masses.