Another way to fix disruptive twinkling is a system called speckle interferometry.
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Speckle interferometry showed in 2009 two almost identical components separated by 0.124 ".
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He also started to work on speckle phenomenon and speckle interferometry using photographic recording.
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In the early 1980s, R136a was first resolved using speckle interferometry into 8 components.
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It has been resolved using speckle interferometry at a distance of 0.25 " in 1972.
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Two stars are only resolved by speckle interferometry.
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This was achieved in 2006 with adaptive optics, and has been achieved since with speckle interferometry.
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In addition, speckle interferometry is realizable under poor atmospheric conditions, while the adaptive optics always needs the best seeing ".
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A third star, revealed by speckle interferometry, is likely to be a cooler star that has evolved off the main sequence.
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This makes it especially useful for tasks such as spectroscopy and speckle interferometry, where light-gathering performance is more important than resolution.
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