CWNU 1298

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0.29 UTI
0.0
CN
0.2
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.0 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.2 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1298 is a sparse, very loose object of high 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, 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– 9.092 62.733 0.354 -2.87 -0.947 –
Hunt & Reffert 2024 9.032 62.75 0.367 -2.879 -0.947 –
Cavallo et al. 2024 9.065 62.7 0.364 – – –
Hunt & Reffert 2023 9.032 62.75 0.367 -2.879 -0.947 –
He et al. 2023 9.132 62.765 0.363 -2.88 -0.932 –

💡 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– 2.59 1.44 1.74 158 0.140 271 – –
Hunt & Reffert 2024 – – – – – 271(1) – –
Cavallo et al. 2024 2.65 1.43 – 158 0.140 – – –
Hunt & Reffert 2023 2.59 1.44 1.74 73 – – – –
He et al. 2023 2.51 1.50 – 355 – – – –

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

Visualization

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