Dolidze 28
Summary
Dolidze 28 is a sparse, very loose object of 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) | 276.371 | -14.656 | – | 0.17 | -1.47 | 0.6 |
| Kharchenko et al. (2012) | 276.37 | -14.65 | – | 0.67 | -3.58 | – |
| Loktin & Popova (2017) | 276.375 | -14.656 | – | -0.305 | -3.775 | 0.6 |
| UCC | 276.378 | -14.665 | 0.395 | -1.716 | -2.709 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.937, Dist=1258.0, Age=8.25 |
| Kharchenko et al. (2012) | e_bv=0.937, distance=1258, log_age=8.25 |
| Loktin & Popova (2017) | E(B-V)=1.614, Dist=4791, logt=7.4 |
Search coordinates in Bayestar19