ESO 429 02

(MWSC 1264)

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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

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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

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 113.349 -28.18 0.312 -2.835 3.671 –
Almeida et al. 2025 113.349 -28.181 – – – –
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 – – –
Hunt & Reffert 2023 113.353 -28.186 0.324 -2.8 3.733 48.07
Just et al. 2023 113.349 -28.188 – – – –
Dias et al. 2021 113.349 -28.181 0.281 -2.806 3.68 –
Loktin & Popova 2017 113.355 -28.19 – -2.81 0.734 –
Kharchenko et al. 2016 113.349 -28.188 – – – –
Dias et al. 2014 113.35 -28.188 – -1.52 -0.56 –
Kharchenko et al. 2013 113.355 -28.19 – -2.15 0.56 –
Dias et al. 2002 113.35 -28.188 – -1.52 -0.56 –

💡 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 – 13 – 187 – –
Hunt & Reffert 2024 – – – – – 748* – –
Cavallo et al. 2024 2.72 1.63 – 13 -0.030 – – –
Hunt & Reffert 2023 2.73 1.51 2.46 22 – – – –
Just et al. 2023 – – – 8 – 214 – –
Dias et al. 2021 2.88 1.23 – 13 -0.120 – – –
Loktin & Popova 2017 1.74 0.16 – 851 – – – –
Kharchenko et al. 2016 2.06 1.29 – 8 – – – –
Kharchenko et al. 2013 2.06 1.29 – 8 – – – –
Dias et al. 2002 1.67 2.79 – 398 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 464 83.9 113.58 -28.12 0.32 -2.83 3.68 93.7 0.23

💡 Note: The % column shows the percentage of members that ESO 429 02 shares with each listed object.

Visualization

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