CWNU 1441

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0.23 UTI
0.0
CN
0.29
Cdens
0.75
CC3
0.06
Clit
1.0
Cdup
Stellar density (N50/rad) 1.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.29 Loose
  • CC3 0.75 High quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

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CWNU 1441 is a sparse, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young 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.

Palma et al. (2025)
Classified as optical pair P99, along with Theia_2007.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (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– 301.661 34.095 0.609 -1.973 -5.333 –
Hunt & Reffert 2024 301.694 34.111 0.615 -1.986 -5.351 –
Cavallo et al. 2024 301.659 34.074 0.617 – – –
Hunt & Reffert 2023 301.694 34.111 0.615 -1.986 -5.351 –
He et al. 2023 301.655 34.069 0.611 -1.993 -5.333 –

💡 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– 1.54 0.72 0.55 48 0.060 89 – –
Hunt & Reffert 2024 – – – – – 89(1) – –
Cavallo et al. 2024 1.46 0.72 – 195 0.060 – – –
Hunt & Reffert 2023 1.54 0.56 0.55 48 – – – –
He et al. 2023 1.58 1.00 – 40 – – – –

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

Visualization

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