Collinder 240
Summary
Collinder 240 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, near 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) | 167.917 | -60.31 | – | -4.33 | -1.82 | -8.02 |
| Loktin & Popova (2017) | 167.91 | -60.309 | – | -4.33 | -1.82 | -8.02 |
| UCC | 168.001 | -60.343 | 0.246 | -6.21 | 2.564 | 42.471 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.31, Dist=1577.0, Age=7.16 |
| Loktin & Popova (2017) | E(B-V)=0.31, Dist=1577, logt=7.16 |
Search coordinates in Bayestar19