NGC 2224
Summary
NGC 2224 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 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) | 96.883 | 12.656 | – | -0.25 | -0.28 | – |
| Loktin & Popova (2017) | 96.885 | 12.657 | – | -0.25 | -0.28 | – |
| UCC | 96.908 | 12.666 | 0.229 | -0.161 | -0.702 | 16.978 |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.0, Dist=2415.0, Age=7.0 |
| Loktin & Popova (2017) | E(B-V)=0.495, Dist=4806, logt=8.95 |
Search coordinates in Bayestar19