CWNU 1497

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0.25 UTI
0.0
CN
0.15
Cdens
0.5
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 0.7 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.15 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1497 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above 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– 70.816 54.906 0.249 0.301 -0.523 –
Zhang et al. 2024 70.798 54.913 – – – –
Hunt & Reffert 2024 70.798 54.913 0.24 0.298 -0.494 –
Cavallo et al. 2024 70.816 54.914 0.237 – – –
Hunt & Reffert 2023 70.798 54.913 0.24 0.298 -0.494 –
He et al. 2023 70.786 54.881 0.254 0.299 -0.505 -30.06

💡 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– 3.31 1.7 1.27 124 -0.036 227 – –
Zhang et al. 2024 – – – – -0.143(1) – – –
Hunt & Reffert 2024 – – – – – 227(1) – –
Cavallo et al. 2024 3.15 1.64 – 102 0.070 – – –
Hunt & Reffert 2023 3.92 1.82 1.27 124 – – – –
He et al. 2023 3.31 1.70 – 501 – – – –

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

Visualization

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