CWNU 148

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0.30 UTI
0.27
CN
0.36
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.8 [N/pc2]
  • CN 0.27 Poorly populated
  • Cdens 0.36 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 148 is a poorly populated, loose object of low 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-rich, intermediate-age cluster (see Parameters). It is poorly studied 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– 358.24 57.762 0.595 -3.524 -1.751 –
Hunt & Reffert 2024 358.319 57.765 0.582 -3.51 -1.723 –
Cavallo et al. 2024 358.257 57.784 0.592 – – –
Hunt & Reffert 2023 358.319 57.765 0.582 -3.51 -1.723 –
He et al. 2022 358.19 57.759 0.6 -3.52 -1.73 –

💡 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– 1.78 1.36 1.07 204 0.834 97 – –
Hunt & Reffert 2024 – – – – – 97(1) – –
Cavallo et al. 2024 1.79 1.24 – 204 0.700 – – –
Hunt & Reffert 2023 1.60 1.36 1.07 162 – – – –
He et al. 2022 1.78 1.38 – 316 0.968 – – –

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

Visualization

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