NGC 2219
Summary
NGC 2219 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, well below the mid-plane. It is poorly 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) | 95.933 | -4.677 | – | -2.92 | -2.93 | – |
| Kharchenko et al. (2012) | 95.933 | -4.695 | – | -1.53 | -1.98 | – |
| Loktin & Popova (2017) | 95.94 | -4.677 | – | -2.92 | -2.93 | – |
| UCC | 95.96 | -4.701 | 0.135 | 0.309 | 0.992 | – |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.4, Dist=2023.0, Age=8.9 |
| Kharchenko et al. (2012) | e_bv=0.521, distance=2325, log_age=8.75 |
| Loktin & Popova (2017) | E(B-V)=0.312, Dist=1799, logt=9.0 |
Search coordinates in Bayestar19