NGC 2165
Summary
NGC 2165 is a sparse, very loose object of intermediate C3 quality. It is located at a moderate distance from the Sun, well 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) | 92.767 | 51.677 | – | -0.11 | -4.04 | – |
| Loktin & Popova (2017) | 92.76 | 51.678 | – | -0.596 | -2.106 | – |
| UCC | 92.755 | 51.706 | 0.204 | -0.518 | -1.092 | -61.621 |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.23, Dist=1445.0, Age=9.18 |
| Loktin & Popova (2017) | E(B-V)=0.426, Dist=2528, logt=9.0 |
Search coordinates in Bayestar19