CWWL 2073

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0.22 UTI
0.0
CN
0.1
Cdens
0.38
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 4.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWWL 2073 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~4.80 kpc) differs significantly from the median photometric distance (~3.60 kpc).

Note: This object shares a moderate percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Distant Low extinction Near-solar metallicity Intermediate age

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 – 116.952 -24.702 0.208 -1.531 1.84 70.755
Hu & Soubiran 2025 116.988 -24.73 – – – –
Hunt & Reffert 2024 116.942 -24.705 0.205 -1.554 1.817 72.326
Cavallo et al. 2024 116.988 -24.73 0.206 – – –
Hunt & Reffert 2023 116.942 -24.705 0.205 -1.554 1.817 72.326
Chi et al. 2023 116.97 -24.682 0.23 -1.512 2.117 –

💡 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 – – – – -0.170* – – –
Hunt & Reffert 2024 – – – – – 157* – –
Cavallo et al. 2024 3.09 1.14 – 550 -0.230 – – –
Hunt & Reffert 2023 4.12 0.56 0.69 558 – – – –
Chi et al. 2023 – – – 600 0.274 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3069 56.0 116.94 -24.7 0.21 -1.54 1.78 – 0.08
CWWL 1438 36.0 116.9 -24.76 0.23 -1.57 1.86 62.24 0.06

💡 Note: The % column shows the percentage of members that CWWL 2073 shares with each listed object.

Visualization

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