Dolidze 40
Summary
Dolidze 40 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, above 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) | 304.483 | 37.933 | – | -0.22 | -0.77 | -8.9 |
| Kharchenko et al. (2012) | 304.485 | 37.875 | – | -5.16 | -2.09 | – |
| Loktin & Popova (2017) | 304.485 | 37.933 | – | -1.279 | -0.783 | -8.9 |
| UCC | 304.463 | 37.88 | 0.257 | -3.558 | -6.467 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.062, Dist=2702.0, Age=8.4 |
| Kharchenko et al. (2012) | e_bv=1.062, distance=2702, log_age=8.4 |
| Loktin & Popova (2017) | E(B-V)=0.539, Dist=2099, logt=7.16 |
Search coordinates in Bayestar19