Ruprecht 95
(OCL 863; ESO 129 30; MWSC 1966)
Summary
Ruprecht 95 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, above 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.
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) | 175.908 | -61.133 | – | -0.82 | -4.0 | – |
| Kharchenko et al. (2012) | 175.912 | -61.155 | – | -4.87 | -3.99 | – |
| Bica et al. (2019) | 175.884 | -61.139 | – | – | – | – |
| UCC | 175.872 | -61.136 | 0.164 | -6.336 | 1.307 | -5.39 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.416, Dist=1634.0, Age=8.495 |
| Kharchenko et al. (2012) | e_bv=0.416, distance=1634, log_age=8.495 |
Search coordinates in Bayestar19