ESO 062 11
(MWSC 1836)
0.21
UTI
0.0
CN
0.06
Cdens
0.62
CC3
0.19
Clit
1.0
Cdup
Nm (P>50%)
18
Core radius and density
2.1 [pc], 0.3 [pc-2]
- CN 0.0 Sparse
- Cdens 0.06 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.19 Rarely studied
- Cdup 1.0 Unique
Overview
ESO 062 11 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature.
(*): The parallax distance estimate (~3.63 kpc) differs significantly from the median photometric distance (~1.80 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 159.734 | -69.028 | 0.275 | -7.106 | 2.571 | -7.987 |
| Just et al. | 2023 | 159.73 | -69.031 | â | â | â | â |
| Bica et al. | 2019 | 159.72 | -69.026 | â | â | â | â |
| Sampedro et al. | 2017 | 159.729 | -69.033 | â | -7.43 | 3.15 | â |
| Kharchenko et al. | 2016 | 159.73 | -69.031 | â | â | â | â |
| Dias et al. | 2014 | 159.729 | -69.033 | â | -7.81 | 2.87 | â |
| Kharchenko et al. | 2013 | 159.735 | -69.035 | â | -8.91 | 6.21 | â |
| Piskunov et al. | 2008 | 159.72 | -69.026 | â | â | â | â |
| Kharchenko et al. | 2005 | 159.73 | -69.03 | â | -13.48 | 3.63 | 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 | 1.8 | 1.38 | â | 1202 | â | 180 | â | â |
| Just et al. | 2023 | â | â | â | 1202 | â | 180 | â | â |
| Kharchenko et al. | 2016 | 2.69 | 1.44 | â | 1202 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.69 | 1.44 | â | 1202 | â | â | â | â |
| Piskunov et al. | 2008 | 0.91 | 1.32 | â | 339 | â | â | â | â |
| Kharchenko et al. | 2005 | 0.91 | 1.32 | â | 339 | â | â | â | â |
MOCA
