CWNU 2304

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0.32 UTI
0.62
CN
0.22
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.1 [N/pc2]
  • CN 0.62 Moderately populated
  • Cdens 0.22 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2304 is a moderately 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, 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– 153.492 -58.335 0.263 -6.985 3.756 0.815
Hunt & Reffert 2024 153.534 -58.321 0.267 -6.974 3.751 -12.369
Cavallo et al. 2024 153.513 -58.308 0.266 – – –
Hunt & Reffert 2023 153.534 -58.321 0.267 -6.974 3.751 -12.369
He et al. 2023 153.554 -58.393 0.277 -7.014 3.772 10.24

💡 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– 3.27 2.06 2.81 105 0.440 550 – –
Hunt & Reffert 2024 – – – – – 550(1) – –
Cavallo et al. 2024 2.83 1.55 – 479 0.440 – – –
Hunt & Reffert 2023 3.27 2.06 2.81 105 – – – –
He et al. 2023 3.39 2.45 – 71 – – – –

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

Visualization

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