Ruprecht 3
Summary
Ruprecht 3 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
This object shares a very small percentage of members with at least one entry reported in the same catalogue.
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) | 100.522 | -29.445 | – | -0.02 | 4.64 | – |
| Angelo et al. (2019) | 100.533 | -29.452 | – | – | – | – |
| UCC | 100.479 | -29.466 | 0.151 | -0.874 | 1.535 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.0, distance=1259, log_age=9.1 |
| Angelo et al. (2019) | dsun=2.29, Age=1.12, Mphot=24 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Ruprecht 2 | 4.0 | 100.3 | -29.51 | 0.12 | -0.47 | 1.79 | 69.32 | 0.08 |