CWNU 2660

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0.58 UTI
0.53
CN
0.98
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 7.2 [arcmin]
  • CN 0.53 Moderately populated
  • Cdens 0.98 Very dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2660 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.
Relatively close High 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 – 278.381 -10.786 0.62 1.073 -2.359 -14.601
Hu & Soubiran 2025 278.354 -10.808 – – – –
Hunt & Reffert 2024 278.377 -10.792 0.634 1.054 -2.362 -22.471
Cavallo et al. 2024 278.354 -10.808 0.631 – – –
Hunt & Reffert 2023 278.377 -10.792 0.634 1.054 -2.362 -22.471
He et al. 2023 278.381 -10.796 0.621 1.071 -2.375 -14.64

💡 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 – – – – 0.040* – – –
Hunt & Reffert 2024 – – – – – 679* – –
Cavallo et al. 2024 1.33 3.98 – 631 -0.200 – – –
Hunt & Reffert 2023 1.52 4.13 2.58 186 – – – –
He et al. 2023 1.51 3.80 – 891 – – – –

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

Visualization

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