NGC 2260
Summary
NGC 2260 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, below 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) | 99.513 | -1.473 | – | -0.64 | -2.1 | – |
| Loktin & Popova (2017) | 99.51 | -1.473 | – | 0.012 | 0.308 | – |
| UCC | 99.575 | -1.524 | 0.11 | -0.215 | 0.473 | – |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.25, Dist=1985.0, Age=7.0 |
| Loktin & Popova (2017) | E(B-V)=0.436, Dist=3333, logt=8.8 |
Search coordinates in Bayestar19