VVV 044
(VVV-CL 044)
0.13
UTI
0.0
CN
0.0
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad)
0.0 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.0 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
VVV 044 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large* distance, near the mid-plane. It is catalogued as a cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.
(*): The parallax distance estimate (~6.72 kpc) differs significantly from the median photometric distance (~11.50 kpc).
Note: This object shares a moderate percentage of members with at least one entry reported in the same catalogue. See table with shared members information.
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 | 226.152 | -58.57 | 0.149 | -6.016 | -3.498 | -56.389 |
| Bica et al. | 2019 | 225.917 | -58.585 | â | â | â | â |
| Morales et al. | 2013 | 225.917 | -58.585 | â | â | â | â |
| Borissova et al. | 2011 | 225.917 | -58.585 | â | â | â | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 11.5 | â | â | â | â | â | â | â |
| Morales et al. | 2013 | 11.50 | â | â | â | â | â | â | â |
MOCA

Morales et al. (2013)
Classified as morphological type 'EC2' (partially embedded cluster). Morphological flag: cluster partially embedded, presence of emission related to PAH or warm dust.