| discov_num | notes | refcode |
| B 1863 | AB + TOK 418AC: B 1863 is a known close binary which has been | |
| unexpectedly found to be a triple. The new distant component C is | ||
| detectable also in the y filter, but we measured only the inner binary | ||
| in y. The star was observed at the Blanco telescope in 2008.5397, and | ||
| the pair actually measured then was AC, at 133.8deg, 0".217, dy =3.7. | ||
| The inner pair AB with a smaller dm was unresolved in 2008.5, while it | ||
| is clearly resolved now. Owing to the large distance from the Sun, we | ||
| expect only a slow motion, so even the inner pair observed since 1929 | ||
| may not yet be ready for computing its first orbit. | 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 |
| idgroup | discov | author |
| 1 | B | van den Bos, W.H. |
| coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
| 17342-1910 | TOK 418 | AC | 2014 | 1 | 134 | 0.2 | 8.70 | 12.00 | F2V | N | 173409.17-191029.6 |
| 17342-1910 | TOK 418 | AC | 2017 | 2 | 133 | 0.2 | 8.70 | 12.00 | F2V | N | 173409.17-191029.6 |
| 17342-1910 | TOK 418 | AC | 2018 | 4 | 137 | 0.2 | 8.70 | 12.00 | F2V | N | 173409.17-191029.6 |
| 17342-1910 | TOK 418 | AC | 2019 | 5 | 137 | 0.2 | 8.70 | 12.00 | F2V | N | 173409.17-191029.6 |