Dolidze 52
Summary
Dolidze 52 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, near 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) | 275.975 | -16.65 | – | 0.75 | -4.21 | – |
| Kharchenko et al. (2012) | 275.981 | -16.64 | – | 1.26 | -6.54 | – |
| Loktin & Popova (2017) | 275.985 | -16.64 | – | 1.297 | -5.319 | – |
| UCC | 276.057 | -16.699 | 0.471 | -1.94 | -2.704 | 4.074 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.625, Dist=1318.0, Age=7.3 |
| Kharchenko et al. (2012) | e_bv=0.625, distance=1318, log_age=7.3 |
| Loktin & Popova (2017) | E(B-V)=0.502, Dist=2079, logt=7.3 |
Search coordinates in Bayestar19