ESO 525 08
(MWSC 3125)
0.14
UTI
0.0
CN
0.01
Cdens
0.12
CC3
0.29
Clit
1.0
Cdup
Nm (P>50%)
20
Core radius and density
11 [pc], 0.04 [pc-2]
- CN 0.0 Sparse
- Cdens 0.01 Very loose
- CC3 0.12 Very low quality
- Clit 0.29 Poorly studied
- Cdup 1.0 Unique
Overview
ESO 525 08 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~7.73 kpc) differs significantly from the median photometric distance (~2.42 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 | 291.844 | -23.576 | 0.129 | -2.517 | -4.297 | 144.67 |
| Just et al. | 2023 | 291.787 | -23.592 | â | â | â | â |
| Bica et al. | 2019 | 291.821 | -23.587 | â | â | â | â |
| Loktin & Popova | 2017 | 291.84 | -23.619 | â | 1.749 | -1.889 | â |
| Sampedro et al. | 2017 | 291.817 | -23.576 | â | 0.85 | -1.27 | â |
| Kharchenko et al. | 2016 | 291.787 | -23.592 | â | â | â | â |
| Tadross | 2014 | 291.817 | -23.576 | â | â | â | â |
| Dias et al. | 2014 | 291.817 | -23.576 | â | 0.99 | -1.43 | â |
| Kharchenko et al. | 2013 | 291.795 | -23.59 | â | -0.14 | -1.58 | â |
| Bukowiecki et al. | 2011 | 291.821 | -23.59 | â | â | â | â |
| Dias et al. | 2002 | 291.817 | -23.576 | â | 0.99 | -1.43 | 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 | 2.415 | 1.31 | â | 1585 | â | 632 | â | â |
| Just et al. | 2023 | â | â | â | 1585 | â | 861 | â | â |
| Loktin & Popova | 2017 | 2.36 | 0.14 | â | 1820 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.57 | 1.51 | â | 1585 | â | â | â | â |
| Tadross | 2014 | 1.64 | 1.14 | â | 1000 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.57 | 1.51 | â | 1585 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 402 | â | â |
| Bukowiecki et al. | 2011 | 2.47(1) | 1.48 | â | 891 | â | â | â | â |
| Dias et al. | 2002 | 1.64 | 1.14 | â | 1000 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA

Dias et al. (2022)
Likely not a real open cluster.