FSR 1470
Summary
FSR 1470 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, well below the mid-plane. It is rarely 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 |
|---|---|---|---|---|---|---|
| Froebrich et al. (2007) | 110.704 | -59.199 | – | – | – | – |
| Kharchenko et al. (2012) | 110.7 | -59.199 | – | -1.89 | 8.19 | – |
| UCC | 110.661 | -59.226 | 0.334 | -2.35 | 7.327 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.416, distance=1055, log_age=8.63 |
Search coordinates in Bayestar19