J05098+2802
This is a quadruple system, consisting of stars named Aa, Ab, B and C. The BC pair is 11" from A, so it should be
possible to shot two different sequences, one for A and another one for BC. The primary component, of mag. 6.0, is a spectroscopic
binary and the separation has reported to be 0.18"; but this has only been observed once (in 1908). A detection based on a
lunar occultation would be most interesting. Components B and C
are separated 0.35" and quite similar in brightness (mags. 9.1 and 9.7). Note that these events are emersions, and the
observations may entail some difficulties.
More information:
www.stelledoppie.it
simbad