Dolidze 18
Summary
Dolidze 18 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 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 |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 80.838 | 33.508 | – | -0.15 | -3.77 | -12.0 |
| Monteiro & Dias (2019) | 80.837 | 33.508 | – | -0.237 | -1.375 | 2.813 |
| UCC | 80.87 | 33.583 | 0.334 | -0.016 | -3.698 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Monteiro & Dias (2019) | E(B-V)=0.478, Dist=3.533, logAge=7.015, Z=0.012 |
Search coordinates in Bayestar19