Waterloo 6
Summary
Waterloo 6 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 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 |
|---|---|---|---|---|---|---|
| Kharchenko et al. (2012) | 130.095 | -46.133 | – | -6.93 | 8.02 | – |
| Loktin & Popova (2017) | 130.095 | -46.132 | – | -7.876 | 3.84 | – |
| UCC | 130.115 | -46.126 | 0.156 | -2.569 | 3.047 | 78.536 |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Kharchenko et al. (2012) | e_bv=0.104, distance=2256, log_age=9.085 |
| Loktin & Popova (2017) | E(B-V)=0.244, Dist=1644, logt=7.695 |
Search coordinates in Bayestar19