VVVX CL009
0.08
UTI
0.0
CN
0.02
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
21.4 [arcmin]
- CN 0.0 Sparse
- Cdens 0.02 Very loose
- CC3 0.38 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
VVVX CL009 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close* distance, above 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 (~1.92 kpc) differs significantly from the median photometric distance (~1.44 kpc).
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 | 191.634 | -60.063 | 0.522 | -6.117 | -0.026 | -28.897 |
| Borissova et al. | 2018 | 191.765 | -60.073 | 0.544 | -6.144 | -0.014 | -4.85 |
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 | 1.44 | â | â | â | â | â | â | â |
Borissova et al. (2018)
Several bright stars, open cluster, IRAS 12441-5947.