discov_num | notes | refcode |
TOK 419 | HIP 85969 has a variable RV according to the GCS and confirmed by | |
Jones et al. (2002 MNRAS 337, 1170). The 0".55 separation implies a | ||
period on the order of 80yr. The star is on the exo-planet program at | ||
the Anglo-Australian Telescope. | 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 |
17342-5454 | TOK 419 | 2014 | 2 | 72 | 0.6 | 7.10 | 11.60 | G4V | 173411.81-545342.2 | ||
17342-5454 | TOK 419 | 2015 | 3 | 73 | 0.6 | 7.10 | 11.60 | G4V | 173411.81-545342.2 | ||
17342-5454 | TOK 419 | 2017 | 4 | 76 | 0.6 | 7.10 | 11.60 | G4V | N | 173411.85-545344.7 | |
17342-5454 | TOK 419 | 2021 | 5 | 82 | 0.6 | 7.10 | 11.60 | G4V | N | 173411.85-545344.7 |