CWNU 1437

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0.50 UTI
0.0
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 12.3 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1437 is a sparse, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young 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– 221.406 -60.986 0.319 -4.895 -2.707 76.051
Hunt & Reffert 2024 221.414 -60.991 0.305 -4.871 -2.694 76.082
Cavallo et al. 2024 221.37 -60.99 0.305 – – –
Hunt & Reffert 2023 221.414 -60.991 0.305 -4.871 -2.694 76.082
He et al. 2023 221.389 -60.988 0.319 -4.902 -2.722 –

💡 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– 3.12 3.94 2.04 8 0.040 623 – –
Hunt & Reffert 2024 – – – – – 623(1) – –
Cavallo et al. 2024 2.39 3.85 – 13 0.040 – – –
Hunt & Reffert 2023 3.12 3.94 2.04 8 – – – –
He et al. 2023 3.55 4.50 – 5 – – – –

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

Visualization

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