FSR 0414
Summary
FSR 0414 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, above 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) | 345.438 | 63.021 | – | 0.11 | -3.8 | -23.0 |
| Froebrich et al. (2007) | 345.438 | 63.021 | – | – | – | – |
| Kharchenko et al. (2012) | 345.435 | 62.983 | – | -1.18 | 0.27 | – |
| UCC | 345.335 | 62.978 | 0.163 | -3.113 | -1.699 | -60.171 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.625, Dist=831.0, Age=8.79 |
| Kharchenko et al. (2012) | e_bv=0.666, distance=957, log_age=8.725 |
Search coordinates in Bayestar19