NGC 2351
Summary
NGC 2351 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near 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) | 108.379 | -10.487 | – | -4.02 | -1.54 | – |
| Kharchenko et al. (2012) | 108.382 | -10.48 | – | -0.43 | 2.54 | – |
| Loktin & Popova (2017) | 108.375 | -10.48 | – | -0.467 | 0.825 | – |
| UCC | 108.398 | -10.451 | 0.229 | -1.232 | 1.524 | 105.237 |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.92, Dist=1882.0, Age=8.38 |
| Kharchenko et al. (2012) | e_bv=0.521, distance=5841, log_age=9.0 |
| Loktin & Popova (2017) | E(B-V)=0.609, Dist=4121, logt=8.79 |
Search coordinates in Bayestar19