| discov_num | notes | refcode |
| JNN 67 | We resolve this star into a close binary (as yet unconfirmed through | |
| common proper motion). It was recently classified as a classical | ||
| Cepheid based on light curve analysis (Christiansen et al. 2008 MNRAS | ||
| 385, 1749). We assume that this is a mis-classification, given that | ||
| the unresolved spectral type is M0.5V. | 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 |
| 09167-2448 | JNN 67 | 2010 | 1 | 161 | 0.1 | 12.20 | 13.10 | M0.5 M2.5 | 091643.98-244742.9 | ||
| 09167-2448 | JNN 67 | 2012 | 2 | 103 | 0.1 | 12.20 | 13.10 | M0.5 M2.5 | NV | 091643.98-244742.9 | |
| 09167-2448 | JNN 67 | 2019 | 7 | 146 | 0.1 | 12.20 | 13.10 | M0.5+M2.5 | NV | 091643.98-244742.9 |