NGC 2013
Summary
NGC 2013 is a poorly populated, very loose object of low C3 quality. It is located at a moderate distance from the Sun, well above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 8 years.
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) | 86.004 | 55.793 | – | 0.51 | -2.81 | – |
| Loktin & Popova (2017) | 86.01 | 55.793 | – | 1.406 | -0.553 | – |
| UCC | 85.98 | 55.823 | 0.268 | 0.708 | -1.353 | 4.886 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.23, Dist=1100.0, Age=9.18 |
| Loktin & Popova (2017) | E(B-V)=0.253, Dist=3141, logt=9.2 |
Search coordinates in Bayestar19