discov_num | notes | refcode |
I 454 | CPD-24@891. C is CPD-24@889. AB,C = LDS 68. | |
AB,C: SHY 135. Bayesian analysis by Shaya & Olling (2011) indicates | Shy2011 | |
very high (near 100%) probability pair is physical. | ||
WSI 7 | Aa,Ab: Tokovinin et al. (2014) derive a combined spectroscopic/ | |
interferometric orbit of the Aa,Ab pair, as well as a new orbit of the | ||
AB pair. Resulting component masses for Aa, Ab, B, and C are 0.74, | ||
0.72, 0.57, and 0.78 Msun, respectively. | Tok2014b |
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.) | ||
Tok2014b | orb - | Tokovinin, A., Gornya, N.A., & Morrell, N.I. | 2014MNRAS.443.3082T |
Tok2014b | MNRAS 443, 3082, 2014 |
idgroup | discov | author |
1 | I | Innes, R.T.A. |
5 | I | MNRAS 57, 533, 1897 (data also in I__1897b, |
5 | I | I__1897c) |
91 | WSI | Douglass, G.G., Hindsley, R.B., & Worley, C.E. |
100 | WSI | Mason, B.D., Hartkopf, W.I., Holdenried, E.R., Rafferty, T.J., Wycoff, G.L., |
100 | WSI | Hennessy, G.S., Hall, D.M., Urban, S.E., et al. |
103 | WSI | Mason, B.D., Hartkopf, W.I., Wycoff, G.L., Holdenried, E.R., Platais, I., |
103 | WSI | Rafferty, T.J., Hall, D.M., Hennessy, G.S., et al. |
104 | WSI | Mason, B.D., Hartkopf, W.I., Urban, S.E., Wycoff, G.L., Pascu, D., Hall, D.M., |
104 | WSI | Hennessy, G.S., Platais, I., et al. |
105 | WSI | Mason, B.D., Hartkopf, W.I., Wycoff, G.L., Pascu, D., Urban, S.E., Hall, D.M., |
105 | WSI | Hennessy, G.S., Rafferty, T.J., et al. |
132 | WSI | Mason, B.D., Hartkopf, W.I., Bredthauer, G., Ferguson, E.W., Finch, C.T., Kilian, |
132 | WSI | C.M., Rafferty, T.J., Ragan, T.J. & Wieder, G.D. |
142 | WSI | Mason, B.D., Williams, S.J., Matson, R.A., Josties, J.D., Eakens, P.D., Justice, |
142 | WSI | M., Kilian, C.M. & Warner, R. |
coord_2000 | discov_num | comp | epoch | obs | pa | sep | mag_pri | mag_sec | spectr | notes | coord_arcsec_2000 |
02057-2423 | I 454 | AB | 1991 | 13 | 146 | 1.2 | 8.68 | 11.44 | K1V | N | 020541.24-242233.2 |
02057-2423 | I 454 | AB | 2008 | 18 | 153 | 0.8 | 8.68 | 11.44 | K1V | N | 020541.24-242233.2 |
02057-2423 | I 454 | AB | 2010 | 22 | 155 | 0.8 | 8.68 | 11.44 | K1V | N | 020541.24-242233.2 |
02057-2423 | I 454 | AB | 2012 | 28 | 157 | 0.7 | 8.68 | 11.44 | K1V | NO | 020541.24-242233.2 |
02057-2423 | I 454 | AB | 2015 | 35 | 159 | 0.7 | 8.62 | 11.32 | G9+G9+K5V | NO | 020541.24-242233.2 |
02057-2423 | I 454 | AB | 2016 | 39 | 159 | 0.6 | 8.62 | 11.32 | G9+G9+K5V | NO | 020541.51-242233.8 |
02057-2423 | I 454 | AB | 2018 | 40 | 162 | 0.6 | 8.62 | 11.32 | G9+G9+K5V | NO | 020541.51-242233.8 |
02057-2423 | I 454 | AB | 2019 | 41 | 164 | 0.6 | 8.62 | 11.32 | G9+G9+K5V | NO | 020541.51-242233.8 |
02057-2423 | I 454 | AB | 2020 | 43 | 166 | 0.5 | 8.62 | 11.32 | G9+G9+K5V | NO | 020541.51-242233.8 |
02057-2423 | I 454 | AB | 2021 | 45 | 166 | 0.5 | 8.62 | 11.32 | G9+G9+K5V | NO | 020541.51-242233.8 |