CWNU 129

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0.33 UTI
0.3
CN
0.49
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 8.7 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.49 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 129 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

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 – 117.545 -34.44 0.721 -4.219 4.205 22.649
Hunt & Reffert 2024 117.59 -34.359 0.705 -4.208 4.23 22.876
Cavallo et al. 2024 117.55 -34.431 0.705 – – –
Hunt & Reffert 2023 117.59 -34.359 0.705 -4.208 4.23 22.876
He et al. 2022 117.468 -34.406 0.71 -4.24 4.21 –

💡 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
Hunt & Reffert 2024 – – – – – 118* – –
Cavallo et al. 2024 1.40 1.66 – 23 -0.080 – – –
Hunt & Reffert 2023 1.37 1.33 1.28 34 – – – –
He et al. 2022 1.29 1.62 – 32 -0.419 – – –

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

Visualization

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