J05098+2802

This is a very interesting star system, with two pairs, A,BC and BC, being physical, and the latter with a known orbit of grade 3. Observation is highly desired. Note that A and BC are widely separated; consider a separate recording if necessary. BC are only at 0.4" but should be detectable if geometry is favourable. A is a spectroscopic binary, but could be at reach for the lunar-occultation technique. Observing conditions should be good.

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