CWNU 388

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0.21 UTI
0.27
CN
0.14
Cdens
0.5
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.9 [pc], 0.7 [pc-2]
  • CN 0.27 Poorly populated
  • Cdens 0.14 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 388 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is rarely studied 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: 0.99 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (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– 307.052 54.449 0.922 -1.736 -6.705 -16.705
Hunt & Reffert 2024 307.105 54.412 0.92 -1.746 -6.657 -4.521
Cavallo et al. 2024 306.727 54.36 0.92 – – –
Hunt & Reffert 2023 307.105 54.412 0.92 -1.746 -6.657 -4.521
He et al. 2022 307.146 54.464 0.92 -1.74 -6.68 –

💡 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– 1.055 0.54 1.59 214 0.190 55 – –
Hunt & Reffert 2024 1.04 0.51 1.59 220 – 55(1) – –
Cavallo et al. 2024 1.12 0.59 – 209 0.260 – – –
Hunt & Reffert 2023 1.04 0.51 1.59 220 – – – –
He et al. 2022 1.07 0.57 – 79 0.119 – – –

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

Visualization

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