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) | ||
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.) |
idgroup | discov | author |
1 | A | Aitken, R.G. |
312 | STF | Struve, F.G.W. |
coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
16579+4722 | A 1874 | AD | 1998 | 2 | 246 | 25.9 | 7.93 | 15.00 | K0 | N W | 165753.18+472200.0 |
16579+4722 | A 1874 | AD | 2000 | 2 | 246 | 25.9 | 7.93 | 15.00 | K0 | 165753.31+472157.7 |