| discov_num | notes | refcode |
| BRT 73 | The 1893 observation differs substantially from modern observations. | |
| Either the 1893 observation is erroneous (which we consider the most | ||
| probable), or there exist perturbations in the system. The question of | ||
| the physical relationship of this system remains open. | Kiy2012 |
| refcode | metd | author | reference |
| Kiy2012 | orb - | Kiyaeva, O.V., Kiselev, A.A., Romanenko, L.G., Kalinichenko, O.A. & Vasileva, T.A. | 2012ARep...56..952K |
| Kiy2012 | ARep 56, 952, 2012 (SvA 89, 1045, 2012) |
| idgroup | discov | author |
| 1 | BRT | Barton, S.G. |
| coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
| 00586+4709 | BRT 73 | 2004 | 3 | 69 | 4.8 | 10.30 | 10.40 | D | 005836.87+470844.4 | ||
| 00586+4709 | BRT 73 | 2006 | 4 | 70 | 4.7 | 10.30 | 10.40 | D | 005836.87+470844.4 | ||
| 00586+4709 | BRT 73 | 2016 | 11 | 70 | 4.7 | 10.30 | 10.40 | N | 005836.87+470844.4 |