CWNU 1292

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0.49 UTI
0.56
CN
0.87
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.4 [N/pc2]
  • CN 0.56 Moderately populated
  • Cdens 0.87 Dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1292 is a moderately populated, dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-poor, very young cluster (see Parameters). It was recently reported in the literature.

Palma et al. (2025)
Classified as optical pair P301, along with HSC_285.

Cavallo et al. (2024)
Silver 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– 281.018 -3.784 0.319 -0.605 -2.591 61.889
Hunt & Reffert 2024 281.043 -3.797 0.313 -0.621 -2.586 45.021
Cavallo et al. 2024 281.013 -3.783 0.312 – – –
Hunt & Reffert 2023 281.043 -3.797 0.313 -0.621 -2.586 45.021
He et al. 2023 281.001 -3.761 0.335 -0.597 -2.565 –

💡 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– 2.87 4.78 2.75 6 -0.930 2482 – –
Hunt & Reffert 2024 – – – – – 2482(1) – –
Cavallo et al. 2024 2.77 4.62 – 32 -0.930 – – –
Hunt & Reffert 2023 2.87 4.78 2.75 6 – – – –
He et al. 2023 3.31 5.15 – 5 – – – –

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

Visualization

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