CWNU 2867

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0.17 UTI
0.0
CN
0.08
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 6.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2867 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Distant High extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 223.235 -60.834 0.325 -4.649 -2.844 -30.762
Hunt & Reffert 2024 223.233 -60.897 0.327 -4.629 -2.844 -10.988
Cavallo et al. 2024 223.122 -60.786 0.329 – – –
Hunt & Reffert 2023 223.233 -60.897 0.327 -4.629 -2.844 -10.988
He et al. 2023 223.226 -60.862 0.331 -4.665 -2.846 –

💡 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 – – – – – 341* – –
Cavallo et al. 2024 3.08 3.76 – 209 -0.010 – – –
Hunt & Reffert 2023 2.69 3.90 2.23 188 – – – –
He et al. 2023 3.31 2.60 – 1 – – – –

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

Visualization

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