Dolidze 24
Summary
Dolidze 24 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) | 101.171 | 1.685 | – | -0.57 | -1.24 | – |
| Kharchenko et al. (2012) | 101.183 | 1.735 | – | -1.46 | -3.12 | – |
| Loktin & Popova (2017) | 101.175 | 1.686 | – | -0.273 | -0.967 | – |
| UCC | 101.188 | 1.731 | 0.213 | -0.705 | 0.259 | 106.65 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.146, Dist=1261.0, Age=8.45 |
| Kharchenko et al. (2012) | e_bv=0.146, distance=1261, log_age=8.45 |
| Loktin & Popova (2017) | E(B-V)=0.182, Dist=3860, logt=8.97 |
Search coordinates in Bayestar19