Ruprecht 124
(OCL 1005; ESO 333 09; MWSC 2602)
Summary
Ruprecht 124 is a sparse, very loose object of intermediate C3 quality. It is located at a very large distance from the Sun, well below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 262.005 | -40.73 | – | -1.77 | -1.88 | – |
| Bica et al. (2019) | 261.979 | -40.719 | – | – | – | – |
| UCC | 261.96 | -40.706 | 0.046 | -4.32 | -7.44 | -80.065 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.937, distance=2186, log_age=8.25 |
Search coordinates in Bayestar19