Waterloo 8
Summary
Waterloo 8 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 rarely studied in the literature, with no articles listed in the last 8 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) | 112.55 | -15.833 | – | -3.21 | 0.64 | – |
| Loktin & Popova (2017) | 112.545 | -15.833 | – | -1.433 | 2.385 | – |
| UCC | 112.556 | -15.817 | 0.16 | -1.324 | 1.451 | 133.206 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Loktin & Popova (2017) | E(B-V)=0.347, Dist=2782, logt=8.99 |
Search coordinates in Bayestar19