discov_num | notes | refcode |
BSO 12 | AB + TOK 410Ba,Bb: HIP 79980 and HIP 79979 form a 23" CPM pair AB | |
where the F6III primary is slightly evolved, while the G1/G2 secondary | ||
is closer to the main sequence, but still above it. The Hipparcos | ||
parallax of B, -4.7mas, is obviously wrong, so we assume the parallax | ||
of the primary, 20.7mas. The RV(B) is variable (GCS), and we resolve | ||
it into a 40mas pair with an estimated period on the order of 1yr. The | ||
pair moved by 10deg in a month. Binary motion is the likely cause of | ||
the incorrect Hipparcos parallax. | Tok2015c | |
TOK 410 | Ba,Bb: SB? | Tok2014d |
refcode | metd | author | reference |
Tok2014d | E2 - | Tokovinin, A. | 2014AJ....147...86T |
Tok2014d | AJ 147, 86, 2014 | ||
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 | BSO | Brisbane Obs. |
coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
16195-3054 | TOK 410 | Ba,Bb | 2014 | 3 | 95 | 0.0 | 7.20 | 8.10 | F9V | N | 161931.48-305406.9 |
16195-3054 | TOK 410 | Ba,Bb | 2015 | 4 | 283 | 0.1 | 7.20 | 8.10 | F9V | N | 161931.48-305406.9 |
16195-3054 | TOK 410 | Ba,Bb | 2017 | 7 | 280 | 0.1 | 7.20 | 8.10 | F9V | N | 161931.48-305406.9 |
16195-3054 | TOK 410 | Ba,Bb | 2018 | 8 | 284 | 0.1 | 7.20 | 8.10 | F9V | N | 161931.48-305406.9 |
16195-3054 | TOK 410 | Ba,Bb | 2019 | 9 | 305 | 0.0 | 7.20 | 8.10 | F9V | N | 161931.48-305406.9 |
16195-3054 | TOK 410 | Ba,Bb | 2020 | 10 | 274 | 0.0 | 7.20 | 8.10 | F9V | N | 161931.48-305406.9 |
16195-3054 | TOK 410 | Ba,Bb | 2021 | 12 | 279 | 0.1 | 7.20 | 8.10 | F9V | N | 161931.48-305406.9 |
16195-3054 | TOK 410 | Ba,Bb | 2022 | 14 | 304 | 0.0 | 7.20 | 8.30 | F9V | NO | 161931.48-305406.9 |