Ruprecht 14
Summary
Ruprecht 14 is a sparse, very loose object of low 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 8 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) | 108.716 | -31.36 | – | -1.26 | 3.53 | – |
| Loktin & Popova (2017) | 108.72 | -31.36 | – | 0.317 | 4.611 | – |
| UCC | 108.776 | -31.367 | 0.06 | -0.766 | 1.793 | 112.882 |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.396, distance=4023, log_age=9.06 |
| Loktin & Popova (2017) | E(B-V)=0.047, Dist=2860, logt=9.19 |
Search coordinates in Bayestar19