NGC 2664
Summary
NGC 2664 is a poorly populated, moderately dense object of very low C3 quality. It is located at a relatively close distance from the Sun, well above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 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 |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 131.843 | 12.6 | – | -7.07 | -4.65 | – |
| UCC | 131.864 | 12.627 | 0.994 | -10.832 | -2.624 | 47.88 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.625, distance=1659, log_age=8.29 |
Search coordinates in Bayestar19