| discov_num |
notes |
refcode |
| A 1874 |
AB: Kiselev et al. derive a family of possible orbital solutions, |
Rmn2009 |
|
based on a range of mass sums (0.93 to 1.53 Msun) and inclinations of |
|
|
the pair to the plane of the sky (-32 to +32deg). |
|
| STFA 32 |
AC: HJL 242. |
HJL1986 |
|
AC: Kiselev et al. derive a family of possible orbital solutions, |
Rmn2009 |
|
based on a range of inclinations of the pair to the plane of the sky |
|
|
(-38 to +38deg). The mass of the AB pair is here assumed to be 1.09 |
|
|
Msun and that of the system 1.89 Msun. |
|
|
AC: SHY 84. Bayesian analysis by Shaya & Olling (2011) indicates very |
Shy2011 |
|
high (near 100%) probability pair is physical. |
|
| refcode |
metd |
author |
reference |
| HJL1986 |
Pa - |
Halbwachs, J.L. |
1986A&AS...66..131H |
| HJL1986 |
|
A&AS 66, 131, 1986 |
|
| HJL1986 |
|
(Possible CPM pairs from AGK2/3. Coarse astrometry, incl. mean 1950 dates, added |
|
| HJL1986 |
|
only for previously unknown pairs. Table 1: HJL 1 - 326, Table 2: HJL1001 - 1113) |
|
| Kis2009b |
Po u |
Kiselev, A.A., Romanenko, L.G. & Gorynya, N.A. |
2009ARep...53.1136K |
| Kis2009b |
|
ARep 53, 1136, 2009 (SvA 86, 1216, 2009) |
|
| 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.) |
|
