| discov_num | notes | refcode |
| JNN 85 | Due to the very compact arrangement of the three components of 2MASS | |
| J13022691-5200507, it is highly probable that this is a physically | ||
| bound triple system. Futhermore, the system is conspicuously close to | ||
| the close binary J13025257-5201384 both on the sky and in distance (52 | ||
| versus 59 pc), hence this is a candidate quintuple system. Only one | ||
| epoch of imaging exists, so common proper motion has not yet been | ||
| demonstrated. | Jnn2012 |
| refcode | metd | author | reference |
| Jnn2012 | Cl j | Janson, M., Hormuth, F., Bergfors, C., Brandner, W., Hippler, S., Daemgen, S., | 2012ApJ...754...44J |
| Jnn2012 | +E2 | Kudryavtseva, N., Schmalzl, E., Schnupp, C., & Henning, T. | |
| Jnn2012 | ApJ 754, 44, 2012 (some recalibrated measures published in Jnn2014b) | 2014ApJS..214...17J |
| coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
| 13024-5201 | JNN 85 | AB | 2010 | 1 | 105 | 0.1 | 13.40 | 14.70 | M2 M4 | 130226.92-520050.6 | |
| 13024-5201 | JNN 85 | AB | 2012 | 2 | 100 | 0.1 | 13.40 | 14.70 | M2 M4 | NV | 130226.92-520050.6 |