| discov_num | notes | refcode |
| TOK 417 | HIP 85963 has a variable RV and is an acceleration binary. The 91mas | |
| separation implies an orbital period of ~10yr; the estimated masses | ||
| are 1.37 and 0.81 Msun. Despite extensive literature (51 references in | ||
| SIMBAD), there is no published spectroscopic orbit, while several | ||
| high-resolution spectroscopic studies addressed the abundance. | Tok2015c |
| refcode | metd | author | reference |
| 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 |
| 17341-0303 | TOK 417 | 2014 | 1 | 89 | 0.1 | 7.50 | 10.00 | F8 | 173408.45-030319.9 | ||
| 17341-0303 | TOK 417 | 2018 | 2 | 2 | 0.0 | 7.50 | 10.00 | F8 | N | 173408.45-030319.9 |