CWNU 2754

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0.18 UTI
0.0
CN
0.02
Cdens
0.75
CC3
0.06
Clit
1.0
Cdup
Core radius and density 3.9 [pc], 0.1 [pc-2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.75 High quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2754 is a sparse, very loose object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD classes: 1.00 (50th percentile), true positive (human-assigned).

Hunt & Reffert (2023)
Classified as open cluster. CMD classes: 1.00 (50th percentile), true 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– 112.932 -14.424 0.357 -1.537 2.121 –
Hunt & Reffert 2024 112.932 -14.458 0.359 -1.542 2.134 –
Cavallo et al. 2024 112.921 -14.432 0.361 – – –
Hunt & Reffert 2023 112.932 -14.458 0.359 -1.542 2.134 –
He et al. 2023 112.905 -14.394 0.365 -1.568 2.116 57.8

💡 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– 2.62 0.6 0.74 127 -0.210 124 – –
Hunt & Reffert 2024 2.52 0.47 0.74 84 – 124(1) – –
Cavallo et al. 2024 2.72 0.73 – 170 -0.210 – – –
Hunt & Reffert 2023 2.52 0.47 0.74 84 – – – –
He et al. 2023 2.95 0.75 – 708 – – – –

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

Visualization

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