NGC 2364
Summary
NGC 2364 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, 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) | 110.192 | -7.55 | – | 0.88 | -2.57 | – |
| Loktin & Popova (2017) | 110.19 | -7.55 | – | -0.435 | 0.341 | – |
| UCC | 110.214 | -7.543 | 0.197 | -0.979 | 0.936 | 79.871 |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.31, Dist=1919.0, Age=8.3 |
| Loktin & Popova (2017) | E(B-V)=0.152, Dist=3788, logt=8.91 |
Search coordinates in Bayestar19