discov_num | notes | refcode |
TOK 44 | Aa,Ab: Tokovinin et al. (2015) derive spectral types G0V and K5V for | |
the Aa and Ab components; masses are 1.46 and 0.64 Msun. Aa is a 170d | ||
SB; Aa2 is possibly of type M3V. | Tok2015b | |
Aa,Ab: SB, P=7.603y. | Tok2014d | |
A 556 | AB: Tokovinin et al. (2015) derives a spectral type K5V for the B | |
component; mass is 0.64 Msun. Dynamical parallax is 27.4 +/- 0.6 mas. | Tok2015b |
refcode | metd | author | reference |
Izm2019 | orb u | Izmailov, I.S. | 2019AstL...45...30I |
Izm2019 | Ast. Lett. 45, 30, 2019 | ||
Izm2019 | (Orbital elements from weighted solutions used when available (Table 2), | ||
Izm2019 | unweighted elements (Table 1) used for remaining 29 systems.) | ||
Tok2014d | E2 - | Tokovinin, A. | 2014AJ....147...86T |
Tok2014d | AJ 147, 86, 2014 | ||
Tok2015b | orb+j | Tokovinin, A., Latham, D.W., & Mason, B.D. | 2015AJ....149..195T |
Tok2015b | +S+ | AJ 149, 195, 2015 |
idgroup | discov | author |
1 | A | Aitken, R.G. |
coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
10370-0850 | TOK 44 | Aa,Ab | 2009 | 1 | 269 | 0.1 | 7.10 | 10.10 | G0 | N | 103700.02-085023.6 |
10370-0850 | TOK 44 | Aa,Ab | 2010 | 4 | 30 | 0.1 | 7.10 | 10.10 | G0 | N D | 103700.02-085023.6 |
10370-0850 | TOK 44 | Aa,Ab | 2012 | 6 | 58 | 0.2 | 7.10 | 10.10 | G0 | N D | 103700.02-085023.6 |
10370-0850 | TOK 44 | Aa,Ab | 2013 | 8 | 84 | 0.1 | 7.10 | 10.10 | G0 | N D | 103700.02-085023.6 |
10370-0850 | TOK 44 | Aa,Ab | 2015 | 13 | 181 | 0.1 | 7.19 | 10.05 | G0V+K5V | NO | 103700.02-085023.6 |
10370-0850 | TOK 44 | Aa,Ab | 2017 | 25 | 245 | 0.1 | 7.19 | 10.05 | G0V+K5V | NO | 103700.02-085023.6 |
10370-0850 | TOK 44 | Aa,Ab | 2018 | 29 | 263 | 0.1 | 7.19 | 10.05 | G0V+K5V | NO | 103700.02-085023.6 |
10370-0850 | TOK 44 | Aa,Ab | 2019 | 32 | 32 | 0.1 | 7.19 | 10.05 | G0V+K5V | NO | 103700.02-085023.6 |
10370-0850 | TOK 44 | Aa,Ab | 2021 | 33 | 62 | 0.1 | 7.19 | 10.05 | G0V+K5V | NO | 103700.02-085023.6 |