CWNU 2467

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0.40 UTI
0.43
CN
0.33
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.5 [arcmin]
  • CN 0.43 Poorly populated
  • Cdens 0.33 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2467 is a poorly populated, loose 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.
Relatively close 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 – 308.102 48.224 0.37 -2.406 -4.736 –
Hunt & Reffert 2024 308.07 48.223 0.366 -2.417 -4.729 –
Cavallo et al. 2024 308.098 48.231 0.367 – – –
Hunt & Reffert 2023 308.07 48.223 0.366 -2.417 -4.729 –
He et al. 2023 308.085 48.186 0.371 -2.406 -4.729 -26.7

💡 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 – – – – – 266* – –
Cavallo et al. 2024 2.92 1.81 – 44 0.290 – – –
Hunt & Reffert 2023 2.52 1.34 2.54 138 – – – –
He et al. 2023 2.45 1.60 – 447 – – – –

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

Visualization

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