This OVRO program "aims at sub-arcsecond resolution corresponding to linear resolutions of 150 to 450 AU." Later, with ALMA, the aim is to achieve "0.1 arcsec resolution, or 15 - 45 AU, close to the peak of the pre-main sequence binary separation distribution."
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*Remember that at 1 kpc, 1000 AU subtends 1 arcsecond.
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