ESO 429 02
(MWSC 1264)
0.61
UTI
0.31
CN
0.7
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
3.2 [arcmin]
- CN 0.31 Poorly populated
- Cdens 0.7 Moderately dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
ESO 429 02 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~3.21 kpc) differs significantly from the median photometric distance (~2.39 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 113.349 | -28.18 | 0.312 | -2.835 | 3.671 | â |
| Almeida et al. | 2025 | 113.349 | -28.181 | â | â | â | â |
| Hunt & Reffert | 2024 | 113.353 | -28.186 | 0.324 | -2.8 | 3.733 | 48.07 |
| Cavallo et al. | 2024 | 113.675 | -27.958 | 0.323 | â | â | â |
| Hunt & Reffert | 2023 | 113.353 | -28.186 | 0.324 | -2.8 | 3.733 | 48.07 |
| Just et al. | 2023 | 113.349 | -28.188 | â | â | â | â |
| Dias et al. | 2021 | 113.349 | -28.181 | 0.281 | -2.806 | 3.68 | â |
| Loktin & Popova | 2017 | 113.355 | -28.19 | â | -2.81 | 0.734 | â |
| Kharchenko et al. | 2016 | 113.349 | -28.188 | â | â | â | â |
| Dias et al. | 2014 | 113.35 | -28.188 | â | -1.52 | -0.56 | â |
| Kharchenko et al. | 2013 | 113.355 | -28.19 | â | -2.15 | 0.56 | â |
| Dias et al. | 2002 | 113.35 | -28.188 | â | -1.52 | -0.56 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.88 | 1.23 | â | 13 | â | 187 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 748* | â | â |
| Cavallo et al. | 2024 | 2.72 | 1.63 | â | 13 | -0.030 | â | â | â |
| Hunt & Reffert | 2023 | 2.73 | 1.51 | 2.46 | 22 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 8 | â | 214 | â | â |
| Dias et al. | 2021 | 2.88 | 1.23 | â | 13 | -0.120 | â | â | â |
| Loktin & Popova | 2017 | 1.74 | 0.16 | â | 851 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.06 | 1.29 | â | 8 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.06 | 1.29 | â | 8 | â | â | â | â |
| Dias et al. | 2002 | 1.67 | 2.79 | â | 398 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.
Cavallo et al. (2024)
Gold sample.