CWNU 1566

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0.09 UTI
0.33
CN
0.5
Cdens
0.38
CC3
0.0
Clit
0.36
Cdup
Stellar density (N50/rad) 2.5 [N/pc2]
  • CN 0.33 Poorly populated
  • Cdens 0.5 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.36 Possibly duplicate

Overview

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CWNU 1566 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, very young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Palma et al. (2025)
Classified as genetic pair P199, along with HSC_860.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.48 (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– 345.852 60.034 0.313 -3.75 -2.759 –
Hunt & Reffert 2024 345.867 60.064 0.319 -3.788 -2.759 –
Cavallo et al. 2024 345.851 60.026 0.317 – – –
Hunt & Reffert 2023 345.867 60.064 0.319 -3.788 -2.759 –
He et al. 2023 345.862 60.031 0.313 -3.75 -2.761 –

💡 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– 3.39 3.24 2.01 16 0.600 225 – –
Hunt & Reffert 2024 – – – – – 225(1) – –
Cavallo et al. 2024 3.94 3.13 – 16 0.600 – – –
Hunt & Reffert 2023 3.10 3.24 2.01 19 – – – –
He et al. 2023 3.39 3.70 – 6 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
BDSB 38 63.6 345.89 60.04 0.31 -3.77 -2.76 – 0.16

💡 Note: The % column shows the percentage of members that CWNU 1566 shares with each listed object.

Visualization

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