CWNU 2585

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0.31 UTI
0.6
CN
0.42
Cdens
0.75
CC3
0.31
Clit
0.65
Cdup
Radius (P>50% members) 6.7 [arcmin]
  • CN 0.6 Moderately populated
  • Cdens 0.42 Loose
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 0.65 Likely unique

Overview

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CWNU 2585 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high 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 was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close High 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 – 358.398 68.232 0.339 -2.828 0.183 -53.82
Hu & Soubiran 2025 358.304 68.242 – – – –
Hunt & Reffert 2024 358.583 68.222 0.334 -2.82 0.163 -52.248
Cavallo et al. 2024 358.304 68.242 0.337 – – –
Hunt & Reffert 2023 358.583 68.222 0.334 -2.82 0.163 -52.248
He et al. 2023 358.414 68.233 0.347 -2.826 0.185 -52.41

💡 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 – – – – 0.000* – – –
Hunt & Reffert 2024 – – – – – 603* – –
Cavallo et al. 2024 2.63 3.68 – 1000 -0.540 – – –
Hunt & Reffert 2023 2.73 3.23 1.42 1346 – – – –
He et al. 2023 2.69 3.10 – 2239 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
PTB 6 34.8 358.15 68.23 0.34 -2.83 0.14 -53.97 0.25

💡 Note: The % column shows the percentage of members that CWNU 2585 shares with each listed object.

Visualization

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