CWNU 1777

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0.21 UTI
0.29
CN
0.2
Cdens
0.38
CC3
0.1
Clit
1.0
Cdup
Core radius and density 1.0 [pc], 1.0 [pc-2]
  • CN 0.29 Poorly populated
  • Cdens 0.2 Very loose
  • CC3 0.38 Low quality
  • Clit 0.1 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1777 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate 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: 0.12 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.12 (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– 243.92 -50.413 0.443 -2.33 -3.921 -81.51
Hu & Soubiran 2025 243.921 -50.396 – – – –
Hunt & Reffert 2024 243.892 -50.37 0.439 -2.336 -3.925 -81.173
Cavallo et al. 2024 243.921 -50.396 0.436 – – –
Hunt & Reffert 2023 243.892 -50.37 0.439 -2.336 -3.925 -81.173
He et al. 2023 243.947 -50.42 0.432 -2.32 -3.921 -81.51

💡 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– 2.2 2.52 1.85 591 0.005 361 – –
Hu & Soubiran 2025 – – – – -0.130(5) – – –
Hunt & Reffert 2024 2.08 2.41 1.85 551 – 361(1) – –
Cavallo et al. 2024 2.32 2.63 – 977 0.140 – – –
Hunt & Reffert 2023 2.08 2.41 1.85 551 – – – –
He et al. 2023 2.51 3.15 – 631 – – – –

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

Visualization

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