discov_num | notes | refcode |
I 1026 | AB + TOK 422Aa,Ab: HIP 91075 was noted as a double-lined binary by | |
the GCS (one observation only). The separation of 86mas implies a | ||
period of ~10yr, while the double-lined observation matches the | ||
moderate magnitude difference (estimated masses 1.04 and 0.77 Msun. | ||
The star is an X-ray source, so a future combined orbit could | ||
determine masses for testing evolutionary models of young stars. The | ||
sky around the object is quite crowded; the 9" companion I 1026 is | ||
optical (it moves too fast). | Tok2015c | |
I 1027 | CD: CPD-27@6461. |
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 |
Tok2021f | orb - | Tokovinin, A. | 2021IAUDS.204....1T |
Tok2021f | Inf. Circ. 204, 1, 2021 |
idgroup | discov | author |
1 | I | Innes, R.T.A. |
5 | I | MNRAS 57, 533, 1897 (data also in I__1897b, |
5 | I | I__1897c) |
coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
18346-2734 | TOK 422 | Aa,Ab | 2014 | 1 | 102 | 0.1 | 9.80 | 11.00 | G3/5V | N | 183437.64-273358.3 |
18346-2734 | TOK 422 | Aa,Ab | 2015 | 3 | 95 | 0.1 | 9.80 | 11.00 | G3/5V | N | 183437.64-273358.3 |
18346-2734 | TOK 422 | Aa,Ab | 2018 | 5 | 107 | 0.1 | 9.80 | 11.00 | G3/5V | N | 183437.64-273358.3 |
18346-2734 | TOK 422 | Aa,Ab | 2019 | 6 | 106 | 0.1 | 9.80 | 11.00 | G3/5V | N | 183437.64-273358.3 |
18346-2734 | TOK 422 | Aa,Ab | 2020 | 7 | 103 | 0.1 | 9.80 | 11.00 | G3/5V | N | 183437.64-273358.3 |
18346-2734 | TOK 422 | Aa,Ab | 2021 | 8 | 102 | 0.1 | 9.80 | 11.00 | G3/5V | N | 183437.64-273358.3 |