CWNU 1504

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0.44 UTI
0.3
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 5.8 [N/pc2]
  • CN 0.3 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1504 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (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– 358.684 60.855 0.398 -1.109 -0.713 86.256
Hunt & Reffert 2024 358.697 60.852 0.402 -1.108 -0.722 –
Cavallo et al. 2024 358.653 60.853 0.402 – – –
Hunt & Reffert 2023 358.697 60.852 0.402 -1.108 -0.722 –
He et al. 2023 358.678 60.852 0.409 -1.104 -0.712 –

💡 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– 2.37 2.08 1.3 242 0.340 175 – –
Hunt & Reffert 2024 – – – – – 175(1) – –
Cavallo et al. 2024 2.75 2.08 – 102 0.340 – – –
Hunt & Reffert 2023 2.37 1.86 1.30 242 – – – –
He et al. 2023 2.24 2.25 – 251 – – – –

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

Visualization

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