Collinder 466
Summary
Collinder 466 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, 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) | 106.733 | -10.715 | – | -0.1 | 0.82 | – |
| Kharchenko et al. (2012) | 106.734 | -10.72 | – | 0.64 | 1.23 | – |
| Loktin & Popova (2017) | 106.74 | -10.73 | – | -0.717 | 0.011 | – |
| UCC | 106.746 | -10.709 | 0.251 | -1.033 | 0.452 | 88.719 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.46, Dist=2123.0, Age=8.8 |
| Kharchenko et al. (2012) | e_bv=0.062, distance=1037, log_age=8.405 |
| Loktin & Popova (2017) | E(B-V)=0.305, Dist=2689, logt=8.93 |
Search coordinates in Bayestar19