Ruprecht 175
Summary
Ruprecht 175 is a sparse, very loose object of 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 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 |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 311.3 | 35.5 | – | -2.6 | -4.4 | – |
| Kharchenko et al. (2012) | 311.265 | 35.503 | – | 0.21 | -3.19 | – |
| Loktin & Popova (2017) | 311.265 | 35.5 | – | -0.297 | -0.94 | – |
| UCC | 311.26 | 35.52 | 0.138 | -1.894 | -2.837 | 14.006 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.521, Dist=4431.0, Age=9.0 |
| Kharchenko et al. (2012) | e_bv=0.521, distance=4431, log_age=9.0 |
| Loktin & Popova (2017) | E(B-V)=0.367, Dist=2932, logt=7.4 |
Search coordinates in Bayestar19