| discov_num | notes | refcode |
| LIM 6 | Liu et al. (2012) derive near-IR spectral types of T8 +/- 0.5 and T9.5 | |
| +/- 0.5. At a derived photometric distance of 19 +/- 3 pc, the two | ||
| stars are separated by 15 +/- 2 au. Various evolutionary models yield | ||
| masses of 19-23 Mjup for the primary, 8.1-10.7 Mjup for the secondary. | LiM2012 |
| refcode | metd | author | reference |
| LiM2012 | Ag j | Liu, M.C., Dupuy, T.J., Bowler, B.P., Leggett, S.K., & Best, W.M.J. | 2012ApJ...758...57L |
| LiM2012 | ApJ 758, 57, 2012 |
| coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
| 17111+3501 | LIM 6 | 2012 | 5 | 328 | 0.8 | 18.30 | 21.38 | T8 T9.5 | N K | 171104.60+350036.8 |