NGC 2314A
(OCl 374; MWSC 1132)
Summary
NGC 2314A is a poorly populated, very loose object of low C3 quality. It is located at a large distance from the Sun, well above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 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) | 107.55 | 75.203 | – | -5.51 | -11.15 | – |
| Bica et al. (2019) | 107.543 | 75.207 | – | – | – | – |
| UCC | 107.557 | 75.22 | 0.195 | 0.222 | 0.083 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.27, Dist=1900.0, Age=7.85 |
Search coordinates in Bayestar19