The optical and radio counterpart of Circinus X-1 (3U 1516 - 56)

Abstract
Circinus X-l (3U 1516 – 56) has a radio counterpart which, at high frequencies, shows flares with the same 16.6-day periodicity as the X-ray intensity. In each cycle the radio flare occurs shortly after the intensity drop-off which defines the X-ray modulation. The radio source is positionally coincident with a faint red star having very strong Hα and weak He I emission lines which are probably variable. The object may be an early-type emission-line star or a symbiotic star, at a distance of 10 kpc.

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