Waterloo 2
Summary
Waterloo 2 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is poorly 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) | 82.004 | 40.372 | – | 0.68 | -0.69 | – |
| Kharchenko et al. (2012) | 82.008 | 40.352 | – | -1.32 | -1.27 | – |
| Loktin & Popova (2017) | 81.99 | 40.353 | – | -0.438 | -0.39 | – |
| UCC | 81.979 | 40.344 | 0.293 | 0.225 | -2.602 | 29.315 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.171, Dist=550.0, Age=8.33 |
| Kharchenko et al. (2012) | e_bv=0.171, distance=550, log_age=8.33 |
| Loktin & Popova (2017) | E(B-V)=0.362, Dist=1995, logt=6.72 |
Search coordinates in Bayestar19