FSR 1412
Summary
FSR 1412 is a sparse, very loose object of very 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 13 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) | 129.287 | -44.153 | – | -3.83 | 7.21 | – |
| Froebrich et al. (2007) | 129.287 | -44.153 | – | – | – | – |
| Kharchenko et al. (2012) | 129.32 | -44.131 | – | -3.83 | 7.21 | – |
| UCC | 129.315 | -44.141 | 0.283 | -3.843 | 3.626 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.208, Dist=2644.0, Age=7.05 |
| Kharchenko et al. (2012) | e_bv=1.208, distance=2644, log_age=7.05 |
Search coordinates in Bayestar19