Ruprecht 110
(OCL 912; ESO 097 10; MWSC 2199)
Summary
Ruprecht 110 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, below the mid-plane. It is poorly studied in the literature, with no articles listed in the last 6 years.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 211.358 | -67.467 | – | -3.6 | -5.01 | -36.65 |
| Piskunov et al. (2007) | 211.36 | -67.468 | – | – | – | – |
| Piskunov et al. (2008) | 211.36 | -67.468 | – | – | – | – |
| Kharchenko et al. (2012) | 211.41 | -67.475 | – | -11.67 | -4.0 | – |
| Bica et al. (2019) | 211.435 | -67.355 | – | – | – | – |
| UCC | 211.35 | -67.388 | 0.193 | -4.161 | -2.822 | -48.811 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.0, Dist=1300.0, Age=8.74, [Fe/H]=-0.359 |
| Piskunov et al. (2007) | E(B-V)=0.0, Dist=1300, logt=8.74, logM=2.365 |
| Piskunov et al. (2008) | E(B-V)=0.0, Dist=1300, logt=8.74, logM=2.947, logMA=2.515 |
| Kharchenko et al. (2012) | e_bv=0.312, distance=1241, log_age=8.7, metallicity=-0.234 |
Search coordinates in Bayestar19