VVV 020
(VVV-CL 020)
0.04
UTI
0.0
CN
0.03
Cdens
0.12
CC3
0.03
Clit
1.0
Cdup
Nm (P>50%)
14
Core radius and density
4.5 [pc], 0.1 [pc-2]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.12 Very low quality
- Clit 0.03 Rarely studied
- Cdup 1.0 Unique
Overview
VVV 020 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 7 years.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 196.901 | -61.301 | 0.39 | -5.483 | -1.394 | -22.023 |
| Bica et al. | 2019 | 196.899 | -61.321 | â | â | â | â |
| Morales et al. | 2013 | 196.9 | -61.324 | â | â | â | â |
| Borissova et al. | 2011 | 196.9 | -61.324 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
MOCA

Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.