J03284+2248Aa,Ab

Double star of uncertain nature, discovered in 1986 and only observed two times since then. The separation is rather small (0.081"). It would be important to confirm duplicity of this star. Given the brightness of the components, high sampling rates are recommended (note that the star is very red, so that use of red or NIR band-pass filters should be considered). The Moon will be very low on the horizon.

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