CWNU 1294

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0.24 UTI
0.37
CN
0.1
Cdens
0.62
CC3
0.06
Clit
1.0
Cdup
Core radius and density 3.9 [pc], 0.5 [pc-2]
  • CN 0.37 Poorly populated
  • Cdens 0.1 Very loose
  • CC3 0.62 Intermediate quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1294 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below 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.

Cavallo et al. (2024)
Silver sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.11 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.11 (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– 259.127 -41.872 0.531 -0.778 -1.069 -7.324
Hunt & Reffert 2024 259.175 -41.875 0.532 -0.788 -1.089 6.176
Cavallo et al. 2024 259.131 -41.847 0.529 – – –
Hunt & Reffert 2023 259.175 -41.875 0.532 -0.788 -1.089 6.176
He et al. 2023 259.103 -41.809 0.533 -0.781 -1.067 -24.8

💡 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– 1.78 3.11 2.415 96 0.230 378 – –
Hunt & Reffert 2024 1.78 3.11 2.41 96 – 378(1) – –
Cavallo et al. 2024 1.91 3.21 – 55 0.230 – – –
Hunt & Reffert 2023 1.78 3.11 2.42 95 – – – –
He et al. 2023 1.70 3.10 – 501 – – – –

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

Visualization

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