FSR 1429
Summary
FSR 1429 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 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) | 129.433 | -46.026 | – | -3.04 | 3.48 | – |
| Froebrich et al. (2007) | 129.433 | -46.026 | – | – | – | – |
| Kharchenko et al. (2012) | 129.41 | -46.017 | – | -3.56 | 9.0 | – |
| UCC | 129.469 | -46.03 | 0.409 | -4.502 | 4.104 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.812, Dist=3371.0, Age=8.2 |
| Kharchenko et al. (2012) | e_bv=0.812, distance=3371, log_age=8.2 |
Search coordinates in Bayestar19