| discov_num | notes | refcode |
| TOK 405 | HIP 67458 is a double-lined chromospherically active binary with | |
| orbital period of 7.2d (Latham, 2012, private communication). We found | ||
| a faint tertiary companion at 0".73 with an estimated orbital period | ||
| on the order of 100yr. The speckle survey of chromospherically active | ||
| stars by Mason et al. (1998) did not detect this tertiary, lacking the | Msn1998b | |
| dynamic range of HRCam. | Tok2015c |
| refcode | metd | author | reference |
| Msn1998b | Sc j | Mason, B.D., Henry, T.J., Hartkopf, W.I., ten Brummelaar, T.A., & Soderblom, D.R. | 1998AJ....116.2975M |
| Msn1998b | AJ 116, 2975, 1998 | ||
| Tok2015c | orb+j | Tokovinin, A., Mason, B.D., Hartkopf, W.I., Mendez, R.A., & Horch, E.P. | 2015AJ....150...50T |
| Tok2015c | +St | AJ 150, 50, 2015 (some measures corrected in Tok2017b) | 2017AJ....154..110T |
| coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
| 13495-2621 | TOK 405 | 2014 | 1 | 15 | 0.7 | 8.00 | 12.00 | G9V | 134927.21-262058.5 | ||
| 13495-2621 | TOK 405 | 2016 | 2 | 14 | 0.7 | 8.00 | 12.00 | G9V | N | 134927.21-262058.5 | |
| 13495-2621 | TOK 405 | 2018 | 8 | 193 | 0.7 | 8.00 | 12.00 | G9V | N | 134927.21-262058.5 | |
| 13495-2621 | TOK 405 | 2019 | 9 | 12 | 0.7 | 8.00 | 12.00 | G9V | N | 134927.21-262058.5 |