Ruprecht 146
(OCL 39; ESO 592 04; MWSC 3012)
Summary
Ruprecht 146 is a sparse, very loose object of very 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.
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) | 283.118 | -21.085 | – | 1.97 | 0.26 | – |
| Bica et al. (2019) | 283.12 | -21.083 | – | – | – | – |
| UCC | 283.073 | -21.09 | 0.181 | -1.839 | -3.9 | -72.103 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.479, distance=1735, log_age=9.1 |
Search coordinates in Bayestar19