CWNU 1392

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0.46 UTI
0.32
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1392 is a poorly populated, very dense 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 (see Parameters). It was recently reported in the literature.
Relatively close Moderate extinction Near-solar metallicity 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 – 71.237 47.911 0.356 0.608 -0.246 -15.73
Hunt & Reffert 2024 71.228 47.912 0.351 0.58 -0.225 -15.962
Cavallo et al. 2024 71.228 47.916 0.351 – – –
Hunt & Reffert 2023 71.228 47.912 0.351 0.58 -0.225 -15.962
He et al. 2023 71.226 47.917 0.368 0.627 -0.229 -18.24

💡 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 – – – – – 436* – –
Cavallo et al. 2024 3.24 3.11 – 479 0.010 – – –
Hunt & Reffert 2023 2.57 2.57 2.09 991 – – – –
He et al. 2023 2.88 2.80 – 1122 – – – –

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

Visualization

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