CWNU 2541

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0.21 UTI
0.42
CN
0.23
Cdens
0.25
CC3
0.06
Clit
1.0
Cdup
Core radius and density 1.8 [pc], 1.1 [pc-2]
  • CN 0.42 Poorly populated
  • Cdens 0.23 Very loose
  • CC3 0.25 Low quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2541 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (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: 0.93 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.93 (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– 334.534 53.731 0.306 -4.097 -4.187 -65.98
Hunt & Reffert 2024 334.537 53.721 0.305 -4.088 -4.169 -65.991
Cavallo et al. 2024 334.623 53.812 0.305 – – –
Hunt & Reffert 2023 334.537 53.721 0.305 -4.088 -4.169 -65.991
He et al. 2023 334.511 53.746 0.322 -4.111 -4.18 -65.98

💡 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– 3.01 1.63 2.43 78 -0.090 213 – –
Hunt & Reffert 2024 3.01 1.26 2.43 78 – 213(1) – –
Cavallo et al. 2024 3.12 2.07 – 51 -0.090 – – –
Hunt & Reffert 2023 3.01 1.26 2.43 78 – – – –
He et al. 2023 2.82 2.00 – 447 – – – –

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

Visualization

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