FSR 0466
Summary
FSR 0466 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, well above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 years.
This object shares a large percentage of members with at least one entry reported in the same catalogue.
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 |
|---|---|---|---|---|---|---|
| Froebrich et al. (2007) | 351.954 | 73.28 | – | – | – | – |
| Kharchenko et al. (2012) | 351.853 | 73.202 | – | -0.17 | 0.36 | – |
| UCC | 351.811 | 73.256 | 0.294 | -3.043 | 0.116 | -56.998 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.812, distance=2227, log_age=8.895 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| FSR 0463 | 76.0 | 351.75 | 73.11 | 0.29 | -3.02 | 0.14 | -57.0 | 0.06 |