Ruprecht 133
Summary
Ruprecht 133 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 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) | 268.121 | -28.667 | – | 0.98 | -2.73 | – |
| Kharchenko et al. (2012) | 268.099 | -28.652 | – | -3.71 | 0.85 | – |
| UCC | 268.171 | -28.664 | 0.118 | -6.034 | -6.692 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.625, Dist=5246.0, Age=8.0 |
| Kharchenko et al. (2012) | e_bv=0.625, distance=5246, log_age=8.0 |
Search coordinates in Bayestar19