| discov_num |
notes |
refcode |
| DUN 10 |
B is CD-51@706. |
|
|
SHY 433. Bayesian analysis by Shaya & Olling (2011) indicates very |
Shy2011 |
|
high (near 100%) probability pair is physical. |
|
|
HIP 14307 and 14313 form a 38" pair belonging to the FG-67 sample. |
|
| TOK 428 |
AC: AC is not co-moving. C=HIP14257 has different parallax |
Tok2014d |
| TOK 428 |
Ba,Bb: The component B is resolved here at 0".19. The estimated |
|
|
period of Ba,Bb is ~25yr. No motion is seen in 2 months. The subsystem |
|
|
Ba,Bb is also manifested by asymmetric line profiles (Tokovinin, in |
|
|
preparation). The A component has never been observed at high angular |
|
|
resolution. |
Tok2015c |
| refcode |
metd |
author |
reference |
| Shy2011 |
- |
Shaya, E.J. & Olling, R. |
2011ApJS..192....2S |
| Shy2011 |
|
ApJS 192, 2, 2011 |
|
| Shy2011 |
|
(Statistical analysis of probability that wide Hipparcos pairs are physical. Pairs |
|
| Shy2011 |
|
added to WDS only if probability 90% or greater.) |
|
| 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 |
| Tok2021c |
orb - |
Tokovinin, A. |
2021IAUDS.203....1S |
| Tok2021c |
|
Inf. Circ. 203, 1, 2021 |
|
