CWNU 2667

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0.59 UTI
0.72
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 1.9 [arcmin]
  • CN 0.72 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2667 is a moderately populated, very dense object of high 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 very small percentage of members with a later reported entry. See table with shared members information.

Distant Moderate 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 – 358.401 63.074 0.255 -3.246 -1.075 -78.558
Hunt & Reffert 2024 358.403 63.071 0.252 -3.233 -1.076 -78.564
Cavallo et al. 2024 358.396 63.071 0.249 – – –
Hunt & Reffert 2023 358.403 63.071 0.252 -3.233 -1.076 -78.564
He et al. 2023 358.391 63.066 0.257 -3.248 -1.097 -78.56

💡 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
Hunt & Reffert 2024 – – – – – 730* – –
Cavallo et al. 2024 3.03 2.25 – 407 -0.330 – – –
Hunt & Reffert 2023 3.64 2.06 1.55 260 – – – –
He et al. 2023 3.55 2.25 – 251 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 10428 1.1 359.0 63.31 0.3 -3.13 -1.09 -5.77 0.08

💡 Note: The % column shows the percentage of members that CWNU 2667 shares with each listed object.

Visualization

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