FSR 1626
(MWSC 2014)
Summary
FSR 1626 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 poorly studied in the literature, with no articles listed in the last 6 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) | 184.971 | -81.499 | – | – | – | – |
| Kharchenko et al. (2012) | 185.025 | -81.51 | – | -6.84 | 1.92 | – |
| Bica et al. (2019) | 184.944 | -81.496 | – | – | – | – |
| UCC | 184.942 | -81.504 | 0.264 | -8.396 | -0.754 | -16.907 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.208, distance=2671, log_age=9.6 |
Search coordinates in Bayestar19