CWNU 7

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0.46 UTI
0.29
CN
1.0
Cdens
0.38
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 7 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Relatively close Low extinction Near-solar metallicity Old

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 – 240.032 -59.103 0.755 -2.697 -1.042 -30.976
Hu & Soubiran 2025 240.061 -59.107 – – – –
Hunt & Reffert 2024 240.093 -59.104 0.759 -2.686 -1.015 -14.689
Cavallo et al. 2024 240.062 -59.107 0.759 – – –
Hunt & Reffert 2023 240.093 -59.104 0.759 -2.686 -1.015 -14.689
He et al. 2022 240.025 -59.095 0.74 -2.72 -1.02 –

💡 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 – – – – -0.290* – – –
Hunt & Reffert 2024 – – – – – 90* – –
Cavallo et al. 2024 1.30 0.18 – 2188 0.440 – – –
Hunt & Reffert 2023 1.25 0.41 0.58 1057 – – – –
He et al. 2022 1.55 0.78 – 251 0.968 – – –

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

Visualization

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