CWNU 2034

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0.15 UTI
0.0
CN
0.12
Cdens
0.5
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.8 [pc], 0.6 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.12 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2034 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 0.12 (50th percentile), false positive? (human-assigned).

Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 0.12 (50th percentile), false positive? (human-assigned).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 325.849 49.619 0.428 -3.634 -3.348 –
Hunt & Reffert 2024 325.88 49.642 0.437 -3.625 -3.345 –
Cavallo et al. 2024 325.885 49.589 0.438 – – –
Hunt & Reffert 2023 325.88 49.642 0.437 -3.625 -3.345 –
He et al. 2023 325.879 49.609 0.438 -3.62 -3.35 –

💡 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– 2.24 2.485 1.76 91 -0.040 220 – –
Hunt & Reffert 2024 2.24 2.34 1.76 91 – 220(1) – –
Cavallo et al. 2024 2.30 2.63 – 79 -0.040 – – –
Hunt & Reffert 2023 2.24 2.34 1.76 91 – – – –
He et al. 2023 2.19 2.80 – 100 – – – –

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

Visualization

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