Dolidze 47
Summary
Dolidze 47 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, below 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) | 310.479 | 36.577 | – | -2.28 | -3.57 | – |
| Kharchenko et al. (2012) | 310.437 | 36.517 | – | -2.0 | -1.23 | – |
| Loktin & Popova (2017) | 310.485 | 36.577 | – | -1.013 | -1.023 | – |
| UCC | 310.496 | 36.529 | 0.226 | -3.443 | -4.894 | -15.192 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.77, Dist=2293.0, Age=8.4 |
| Kharchenko et al. (2012) | e_bv=0.77, distance=2293, log_age=8.4 |
| Loktin & Popova (2017) | E(B-V)=0.123, Dist=1986, logt=9.16 |
Search coordinates in Bayestar19