HU 304 AB: 508; 850x: Suspected not single at lower powers, the equal white stars was a clean split at 850x on up through 1270x, with apodizing mask. I could not tell which star was brighter, but the position angle was following a NE-SW line. It gave me less trouble than I expexted since brighter pairs throw off a lot of diffraction. Pretty cool that this pair, discovered in 1901 at 0.3" and with a 54.7-year period, has made a little more than two complete revolutions to be resolved visually again. WDS grade 2 orbit, no reason to doubt it, and anyway there's no Gaia parallax data available.
04h 23m 51.84s +09° 27' 39.5" P.A. 38.30 sep 0.31" mag 5.80,5.90 Sp A0V+A1V dist. 121.36 pc (395.88 l.y.)
BU1007 AB: 508; 1270x: Snowman, 1 Dm, very tough, broken up with diffraction, PA to the south. Actual PA more WSW, and a WDS grade 2 orbit 111.02-year period. No Gaia data for the secondary. This will become undetectible until the late 2050s. Burnham writes: "Discovered with the 12-inch on Mt. Hamilton in 1881. It was single or too close for the 36-inch 1890-92. The measures since then show but little change in the angle, but a while revolution may be covered by the observations. The components are nearly equal, and therefore some of the measures may require a correction 180 degrees. In my measure with the 40-inch in 1897 it was noted: 'The distance is less than 0.3"; the smaller star is p.' In the first set of measures in 1881 with the 12-inch it was stated: 'The measured distances are decidely too large.' The distance is probably always less than 0.25". There is little double of its being a binary of short period."
STT 79 AB: 508; 570x: Very pretty light orange primary, grey-blue B, 1 Dm, nice close split, PA to north. WDS grade 2 orbit, 89.7-year period, no Gaia data for the secondary. This will widen slightly and be more firmly to the northeast by 2040.
I made an attempt at A3010, and thought I had an elongation with north-south PA, but it is really to the east and I obviously did not have it. Discovered in 1901 at 0.1", it has an extrodinary fast 1.19-year period with a grade 3 orbit. The nice thing is this will be at apistron just next year, so I can certainly give it another go.
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