VVV 136
(VVV-CL 136)
Summary
VVV 136 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 small 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) | 265.738 | -29.882 | – | – | – | – |
| UCC | 265.727 | -29.837 | 0.516 | -1.374 | -1.45 | 13.93 |
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 132 | 12.0 | 265.33 | -29.7 | 0.53 | -1.03 | -1.55 | -55.71 | 0.06 |
| VVV 133 | 12.0 | 265.38 | -29.73 | 0.49 | -1.18 | -1.65 | -34.85 | 0.09 |
| Ryu 524 | 4.0 | 265.68 | -30.1 | 0.39 | -0.66 | -1.12 | 108.05 | 0.33 |