VVVX CL080
0.09
UTI
0.0
CN
0.07
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
10.4 [arcmin]
- CN 0.0 Sparse
- Cdens 0.07 Very loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
VVVX CL080 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close* 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 8 years.
(*): The parallax distance estimate (~1.95 kpc) differs significantly from the median photometric distance (~1.20 kpc).
Note: This object shares a small 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.
Relatively close
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 273.565 | -17.886 | 0.513 | -0.189 | -3.16 | -4.381 |
| Borissova et al. | 2018 | 273.527 | -17.935 | 0.534 | -0.157 | -3.113 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Borissova et al. | 2018 | 1.20 | â | â | â | â | â | â | â |
Borissova et al. (2018)
Small group around B0V star [MCF2015] 13, neb, concentrated.