CWNU 2661

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0.34 UTI
0.75
CN
0.23
Cdens
0.5
CC3
0.1
Clit
1.0
Cdup
Core radius and density 3.4 [pc], 1.2 [pc-2]
  • CN 0.75 Rich
  • Cdens 0.23 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 2661 is a rich, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.60 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.60 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 122.509 -29.85 0.205 -2.789 2.63 58.825
Hu & Soubiran 2025 122.493 -29.849 – – – –
Hunt & Reffert 2024 122.503 -29.854 0.214 -2.785 2.626 62.673
Cavallo et al. 2024 122.493 -29.849 0.212 – – –
Hunt & Reffert 2023 122.503 -29.854 0.214 -2.785 2.626 62.673
He et al. 2023 122.504 -29.837 0.213 -2.792 2.614 59.79

💡 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] Bfrac BSS
UCC 99999– 4.31 1.305 2.03 862 -0.275 866 – –
Hu & Soubiran 2025 – – – – -0.260(5) – – –
Hunt & Reffert 2024 4.31 1.18 2.03 862 – 866(1) – –
Cavallo et al. 2024 3.55 1.43 – 1122 -0.290 – – –
Hunt & Reffert 2023 4.31 1.18 2.03 861 – – – –
He et al. 2023 5.13 1.80 – 501 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 2701 62.6 122.51 -29.85 0.2 -2.77 2.6 59.57 0.04

💡 Note: The % column shows the percentage of members that CWNU 2661 shares with each listed object.

Visualization

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