Czernik 11
Summary
Czernik 11 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 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) | 39.146 | 59.633 | – | -0.08 | -0.53 | – |
| Loktin & Popova (2017) | 39.135 | 59.632 | – | -1.123 | -4.417 | – |
| UCC | 39.189 | 59.637 | 0.303 | -0.606 | -0.092 | -50.779 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.0, Dist=1210.0, Age=8.54 |
| Loktin & Popova (2017) | E(B-V)=1.461, Dist=2346, logt=8.0 |
Search coordinates in Bayestar19