| discov_num | notes | refcode |
| JNN 126 | LP 636-19. | |
| The M3.0 equal-flux binary was first resolved by Janson et al. (2012), | Jnn2012 | |
| and has seen significant orbital motion. Its parallactic distance of | ||
| 37.9 +/- 5.7 pc (Shkolnik et al. 2012 ApJ 758, 56) implies a physical | ||
| separation of ~3-5 au. The expected orbital period is 10-20y. | Bwl2015 |
| refcode | metd | author | reference |
| Bwl2015 | Ac j | Bowler, B.P., Liu, M.C., Shkolnik, E.L., & Tamura, M. | 2015ApJS..216....7B |
| Bwl2015 | ApJS 216, 7, 2015 | ||
| 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 |
| 20532-0221 | JNN 126 | 2008 | 1 | 321 | 0.1 | 13.50 | 14.90 | M3 M4 | N | 205314.66-022121.9 | |
| 20532-0221 | JNN 126 | 2010 | 2 | 327 | 0.1 | 13.50 | 14.90 | M3 M4 | N | 205314.66-022121.9 |