CWNU 2890

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0.20 UTI
0.0
CN
0.39
Cdens
0.5
CC3
0.06
Clit
1.0
Cdup
Core radius and density 0.9 [pc], 1.9 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.39 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2890 is a sparse, loose object of intermediate 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, young cluster, but with a large variance across recent sources for the age parameter (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.

Palma et al. (2025)
Classified as optical pair P365, along with UFMG_82.

Cavallo et al. (2024)
Silver sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.41 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.41 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 262.398 -34.329 0.606 1.976 0.163 112.425
Hunt & Reffert 2024 262.423 -34.321 0.599 1.873 0.176 112.443
Cavallo et al. 2024 262.387 -34.321 0.597 – – –
Hunt & Reffert 2023 262.423 -34.321 0.599 1.873 0.176 112.443
He et al. 2023 262.41 -34.314 0.614 1.968 0.218 –

💡 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] Bfrac BSS
UCC 99999– 1.58 4.22 2.55 86 -0.300 297 – –
Hunt & Reffert 2024 1.58 4.07 2.55 30 – 297(1) – –
Cavallo et al. 2024 1.86 4.37 – 141 -0.300 – – –
Hunt & Reffert 2023 1.58 4.07 2.55 30 – – – –
He et al. 2023 1.51 4.60 – 158 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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