CWNU 2575

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0.21 UTI
0.39
CN
0.04
Cdens
0.5
CC3
0.06
Clit
1.0
Cdup
Core radius and density 6.4 [pc], 0.2 [pc-2]
  • CN 0.39 Poorly populated
  • Cdens 0.04 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.06 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 2575 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate 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)
Part of multiple system G47, along with CWNU_1962 and CWNU_2736.

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

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 108.933 -10.597 0.329 -1.368 1.443 –
Hunt & Reffert 2024 109.019 -10.614 0.32 -1.37 1.451 –
Cavallo et al. 2024 108.905 -10.6 0.321 – – –
Hunt & Reffert 2023 109.019 -10.614 0.32 -1.37 1.451 –
He et al. 2023 108.894 -10.598 0.339 -1.377 1.444 123.37

💡 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– 2.71 1.81 0.7 31 -0.040 300 – –
Hunt & Reffert 2024 2.79 1.81 0.70 31 – 300(1) – –
Cavallo et al. 2024 2.41 1.81 – 35 -0.040 – – –
Hunt & Reffert 2023 2.79 1.81 0.70 31 – – – –
He et al. 2023 2.63 2.00 – 25 – – – –

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

Visualization

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