CWNU 339

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0.29 UTI
0.25
CN
0.32
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 8.7 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.32 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 339 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 – 125.935 -43.025 0.639 -3.922 2.742 1.869
Hunt & Reffert 2024 125.862 -42.985 0.637 -3.925 2.735 1.976
Cavallo et al. 2024 125.905 -43.042 0.641 – – –
Hunt & Reffert 2023 125.862 -42.985 0.637 -3.925 2.735 1.976
He et al. 2022 125.924 -43.094 0.64 -3.95 2.74 17.1

💡 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 – – – – – 80* – –
Cavallo et al. 2024 1.40 1.23 – 93 -0.330 – – –
Hunt & Reffert 2023 1.50 0.87 0.70 92 – – – –
He et al. 2022 1.82 1.14 – 126 0.968 – – –

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

Visualization

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