ESO 429 05
(MWSC 1282)
0.74
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Radius (P>50% members)
1.4 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
ESO 429 05 is a rich, very dense object of high C3 quality. Its parallax locates it at a large* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~9.90 kpc) differs significantly from the median photometric distance (~5.22 kpc).
Very distant
Moderate extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 114.257 | -32.204 | 0.101 | -1.496 | 1.718 | 64.772 |
| Hu & Soubiran | 2025 | 114.27 | -32.21 | â | â | â | â |
| Hunt & Reffert | 2024 | 114.255 | -32.203 | 0.089 | -1.49 | 1.675 | 65.193 |
| Cavallo et al. | 2024 | 114.27 | -32.21 | 0.083 | â | â | â |
| He et al. | 2023 | 114.258 | -32.202 | 0.088 | -1.507 | 1.674 | 64.77 |
| Hunt & Reffert | 2023 | 114.255 | -32.203 | 0.089 | -1.49 | 1.675 | 65.193 |
| Just et al. | 2023 | 114.257 | -32.203 | â | â | â | â |
| Bica et al. | 2019 | 114.259 | -32.197 | â | â | â | â |
| Kharchenko et al. | 2016 | 114.257 | -32.203 | â | â | â | â |
| Kharchenko et al. | 2013 | 114.262 | -32.205 | â | -1.6 | 7.71 | â |
| Dias et al. | 2002 | 114.258 | -32.198 | â | 1.7 | 4.45 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.040* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 608* | â | â |
| Cavallo et al. | 2024 | 6.55 | 1.43 | â | 10965 | -0.390 | â | â | â |
| He et al. | 2023 | 6.46 | 1.45 | â | 6310 | â | â | â | â |
| Hunt & Reffert | 2023 | 9.04 | 2.21 | 1.27 | 940 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1230 | â | 128 | â | â |
| Kharchenko et al. | 2016 | 3.98 | 2.90 | â | 1230 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.98 | 2.90 | â | 1230 | â | â | â | â |
| Dias et al. | 2002 | 3.60 | 2.51 | â | 1259 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.