VVV 140
(VVV-CL 140)
Summary
VVV 140 is a sparse, very loose object of very low C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
This object shares a large percentage of members with at least one entry reported in the same catalogue.
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 |
|---|---|---|---|---|---|---|
| Bica et al. (2019) | 265.969 | -31.731 | – | – | – | – |
| UCC | 265.945 | -31.678 | 0.502 | -0.681 | -0.96 | -28.782 |
Estimated members
Explore data in Colab
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| VVV 139 | 88.0 | 265.93 | -31.68 | 0.5 | -0.63 | -0.97 | -28.78 | 0.09 |
| Ryu 513 | 12.0 | 265.83 | -31.66 | 0.41 | -0.9 | -1.8 | -0.59 | 0.32 |