FSR 1390
Summary
FSR 1390 is a poorly populated, very loose object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is poorly studied in the literature, with no articles listed in the last 13 years.
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) | 127.092 | -40.085 | – | -2.93 | 4.0 | – |
| Froebrich et al. (2007) | 127.092 | -40.085 | – | – | – | – |
| Kharchenko et al. (2012) | 127.092 | -40.083 | – | -2.93 | 4.0 | – |
| UCC | 127.051 | -40.084 | 0.202 | -3.302 | 4.022 | 70.725 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.249, Dist=2397.0, Age=8.3 |
| Kharchenko et al. (2012) | e_bv=1.249, distance=2397, log_age=8.3 |
Search coordinates in Bayestar19