ESO 561 05
(MWSC 1402)
0.16
UTI
0.0
CN
0.03
Cdens
0.12
CC3
0.32
Clit
1.0
Cdup
Nm (P>50%)
20
Core radius and density
2.6 [pc], 0.1 [pc-2]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.12 Very low quality
- Clit 0.32 Poorly studied
- Cdup 1.0 Unique
Overview
ESO 561 05 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~4.23 kpc) differs significantly from the median photometric distance (~2.77 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 | 119.824 | -22.717 | 0.236 | -2.366 | 1.888 | 89.143 |
| Just et al. | 2023 | 119.823 | -22.687 | â | â | â | â |
| Bica et al. | 2019 | 119.821 | -22.689 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -2.92 | 1.66 | â |
| Dib et al. | 2018 | 119.829 | -22.69 | â | â | â | â |
| Loktin & Popova | 2017 | 119.835 | -22.692 | â | -0.334 | 3.581 | â |
| Sampedro et al. | 2017 | 119.829 | -22.692 | â | -3.63 | 3.14 | â |
| Kharchenko et al. | 2016 | 119.823 | -22.687 | â | â | â | â |
| Dias et al. | 2014 | 119.829 | -22.692 | â | -3.58 | 3.85 | â |
| Kharchenko et al. | 2013 | 119.829 | -22.69 | â | 1.11 | 3.79 | â |
| Bukowiecki et al. | 2011 | 119.825 | -22.696 | â | â | â | â |
| Dias et al. | 2002 | 119.829 | -22.692 | â | -3.58 | 3.85 | 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 | 2.77 | 0.46 | â | 1000 | â | 312 | â | â |
| Just et al. | 2023 | â | â | â | 1000 | â | 265 | â | â |
| Dib et al. | 2018 | 1.86 | â | â | 1000 | â | â | â | â |
| Loktin & Popova | 2017 | 4.24 | 0.00 | â | 832 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.86 | 0.46 | â | 1000 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.86 | 0.46 | â | 1000 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 358 | â | â |
| Bukowiecki et al. | 2011 | 3.69(1) | 1.14 | â | 224 | â | â | â | â |
| Dias et al. | 2002 | 3.68 | 1.17 | â | 224 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA
