Speckle Interferometric Observation of WDS 14564$+$8503

Speckle interferometric observations of tertiary star system WDS 14564$+$8503 were made in order to measure the position angle (theta) and separation (rho) of the AB components, and also to attempt to confirm if the components are in a gravitationally bound state. The theta and rho measurements were found to be 291.5\textdegree $+$/- 0.1\textordmasculine and 3.433'' $+$/- 0.01'', respectively. The measurements showed a possible continuation of a linear motion trend, but were inconclusive in confirming whether or not the AB components are gravitationally bound.