FSR 1767
Summary
FSR 1767 is a sparse, very loose object of low C3 quality. It is located at a large 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) | 263.929 | -36.358 | – | 1.4 | -1.98 | – |
| Froebrich et al. (2007) | 263.929 | -36.358 | – | – | – | – |
| Kharchenko et al. (2012) | 263.925 | -36.355 | – | 0.97 | -3.57 | – |
| UCC | 263.944 | -36.316 | 0.177 | -3.942 | -4.691 | -134.021 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.405, Dist=1948.0, Age=8.675 |
| Kharchenko et al. (2012) | e_bv=1.405, distance=1948, log_age=8.675 |
Search coordinates in Bayestar19