VVV 011
(VVV-CL 011)
Summary
VVV 011 is a sparse, very loose object of low C3 quality. It is located at a very large distance from the Sun, below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.88) 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 |
|---|---|---|---|---|---|---|
| Borissova et al. (2011) | 183.171 | -62.709 | – | – | – | – |
| Bica et al. (2019) | 183.179 | -62.709 | – | – | – | – |
| UCC | 183.211 | -62.71 | 0.032 | -6.298 | 0.568 | – |
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 |
|---|---|---|---|---|---|---|---|---|
| CWNU 3471 | 16.0 | 183.26 | -62.71 | 0.17 | -6.25 | 0.64 | 10.87 | 0.19 |
| Alessi 52 | 12.0 | 183.14 | -62.7 | 0.14 | -6.36 | 0.69 | – | 0.16 |
| CWNU 3697 | 4.0 | 182.98 | -62.65 | 0.19 | -6.36 | 0.67 | – | 0.06 |