Answers are grounded in this paper and cite their sources.
We present speckle observations of nineteen double stars and the triple star 2 Cam. Angular separations, absolute position angles and relative photometry result from these observations. The angular separation is derived from the power spectrum. The position angle and the relative photometry are determined by two recent techniques: the cross-correlation between the speckle images and their square, and the ratios of twofold probability density functions of the images.
No takes yet. Share an insight, caveat, or question.
Aristidi et al. (1997) studied this question.
Synapse has enriched 5 related papers. Consider them for comparative context: