CWNU 151

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0.55 UTI
0.26
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 11.4 [N/pc2]
  • CN 0.26 Poorly populated
  • 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 151 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

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– 266.462 -33.457 0.579 1.678 -1.212 –
Hunt & Reffert 2024 266.475 -33.443 0.572 1.632 -1.197 –
Cavallo et al. 2024 266.456 -33.478 0.573 – – –
Hunt & Reffert 2023 266.475 -33.443 0.572 1.632 -1.197 –
He et al. 2022 266.438 -33.481 0.57 1.68 -1.2 –

💡 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– 1.41 1.8 0.38 63 -0.650 242 – –
Hunt & Reffert 2024 – – – – – 242(1) – –
Cavallo et al. 2024 1.18 2.76 – 46 -1.470 – – –
Hunt & Reffert 2023 1.63 1.64 0.38 63 – – – –
He et al. 2022 1.41 1.80 – 158 0.169 – – –

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

Visualization

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