VVV 132

(VVV-CL 132)

Click to load Aladin Lite
UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.15 0.12 0.0 1.0
C3
N_50
r_50
DC 15 8.1
Summary

VVV 132 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 moderate 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.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Bica et al. (2019) 265.406 -29.739 – – – –
           
UCC 265.33 -29.701 0.533 -1.026 -1.554 -55.705
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

VVV 132 UCC

Explore data in Colab

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
VVV 133 44.0 265.38 -29.73 0.49 -1.18 -1.65 -34.85 0.09
VVV 136 12.0 265.73 -29.84 0.52 -1.37 -1.45 13.93 0.05