CWNU 1968

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0.31 UTI
0.0
CN
0.69
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.69 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1968 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Metal-poor Intermediate age

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 – 276.934 -14.074 0.485 -0.565 -0.778 -9.729
Hunt & Reffert 2024 276.899 -14.035 0.494 -0.543 -0.722 –
Cavallo et al. 2024 276.917 -14.062 0.494 – – –
Hunt & Reffert 2023 276.899 -14.035 0.494 -0.543 -0.722 –
He et al. 2023 276.941 -14.102 0.49 -0.562 -0.783 -24.47

💡 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 173* – –
Cavallo et al. 2024 1.27 2.79 – 324 -0.580 – – –
Hunt & Reffert 2023 1.89 2.42 0.85 147 – – – –
He et al. 2023 1.95 2.65 – 398 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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