Ruprecht 114
Summary
Ruprecht 114 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 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 |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 241.583 | -56.867 | – | -4.53 | -4.96 | – |
| Kharchenko et al. (2012) | 241.584 | -56.867 | – | 0.99 | 0.23 | – |
| UCC | 241.469 | -56.899 | 0.287 | -3.723 | -5.023 | -59.148 |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.625, Dist=2088.0, Age=8.9 |
| Kharchenko et al. (2012) | e_bv=0.625, distance=2088, log_age=8.9 |
Search coordinates in Bayestar19