CWNU 2574

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0.56 UTI
0.43
CN
0.86
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.3 [N/pc2]
  • CN 0.43 Poorly populated
  • Cdens 0.86 Dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2574 is a poorly populated, dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as an extremely metal-poor, young cluster (see Parameters). It was recently reported in the literature.

Palma et al. (2025)
Part of multiple system G53, along with CWNU_2470 and HSC_202.

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 277.23 -12.945 0.542 -0.405 -2.585 –
Hunt & Reffert 2024 277.212 -12.947 0.539 -0.413 -2.615 17.608
Cavallo et al. 2024 277.207 -12.956 0.539 – – –
Hunt & Reffert 2023 277.212 -12.947 0.539 -0.413 -2.615 17.608
He et al. 2023 277.201 -12.969 0.538 -0.412 -2.59 –

💡 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– 1.7 2.35 1.37 48 -2.100 313 – –
Hunt & Reffert 2024 – – – – – 313(1) – –
Cavallo et al. 2024 2.08 2.81 – 48 -2.100 – – –
Hunt & Reffert 2023 1.70 2.16 1.37 48 – – – –
He et al. 2023 1.66 2.35 – 22 – – – –

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

Visualization

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