NGC 2239
Summary
NGC 2239 is a poorly populated, very dense object of high C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 8 years.
This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 97.737 | 4.969 | – | -0.6 | -2.18 | – |
| Loktin & Popova (2017) | 97.74 | 4.97 | – | -0.6 | -2.18 | – |
| UCC | 97.756 | 4.939 | 0.673 | -1.834 | 0.029 | 24.063 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.1, Dist=3900.0, Age=6.7 |
| Loktin & Popova (2017) | E(B-V)=0.814, Dist=3116, logt=8.78 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| NGC 2244 | 31.9 | 98.01 | 4.91 | 0.65 | -1.71 | 0.23 | 27.15 | 0.93 |