CWNU 1352

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0.21 UTI
0.3
CN
0.22
Cdens
0.38
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.2 [pc], 1.1 [pc-2]
  • CN 0.3 Poorly populated
  • Cdens 0.22 Very loose
  • CC3 0.38 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1352 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate 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.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.92 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.92 (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– 326.751 54.18 0.592 -2.545 -1.811 -28.233
Hunt & Reffert 2024 326.743 54.187 0.593 -2.518 -1.782 –
Cavallo et al. 2024 326.797 54.165 0.593 – – –
Hunt & Reffert 2023 326.743 54.187 0.593 -2.518 -1.782 –
He et al. 2023 326.781 54.186 0.595 -2.51 -1.811 -22.41

💡 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– 1.65 2.56 1.22 236 0.460 172 – –
Hunt & Reffert 2024 1.65 2.56 1.22 185 – 172(1) – –
Cavallo et al. 2024 1.69 2.38 – 288 0.460 – – –
Hunt & Reffert 2023 1.65 2.56 1.22 185 – – – –
He et al. 2023 1.62 2.60 – 447 – – – –

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

Visualization

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