NGC 2189
(MWSC 788)
Summary
NGC 2189 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 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 |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 93.03 | 1.055 | – | 1.88 | -2.16 | – |
| Bica et al. (2019) | 93.08 | 1.136 | – | – | – | – |
| UCC | 93.067 | 1.083 | 0.336 | -0.159 | -1.942 | 31.802 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.208, distance=1468, log_age=9.175 |
Search coordinates in Bayestar19