CWNU 1885

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0.30 UTI
0.26
CN
0.25
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.2 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.25 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1885 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

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– 351.568 62.009 0.504 -2.48 -1.341 –
Hunt & Reffert 2024 351.514 61.984 0.518 -2.474 -1.339 –
Cavallo et al. 2024 351.544 62.004 0.515 – – –
Hunt & Reffert 2023 351.514 61.984 0.518 -2.474 -1.339 –
He et al. 2023 351.518 62.013 0.524 -2.474 -1.336 –

💡 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– 1.91 2.99 1.43 107 0.340 132 – –
Hunt & Reffert 2024 – – – – – 132(1) – –
Cavallo et al. 2024 1.91 2.99 – 107 0.340 – – –
Hunt & Reffert 2023 1.87 2.99 1.43 124 – – – –
He et al. 2023 2.00 1.30 – 2 – – – –

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

Visualization

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