CWNU 144

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0.38 UTI
0.45
CN
0.21
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 17.0 [arcmin]
  • CN 0.45 Poorly populated
  • Cdens 0.21 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 144 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Relatively close Low 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 – 331.944 50.8 0.76 1.945 -0.398 -21.296
Hunt & Reffert 2024 332.294 50.897 0.773 1.984 -0.437 -15.945
Cavallo et al. 2024 331.507 50.511 0.774 – – –
Hunt & Reffert 2023 332.294 50.897 0.773 1.984 -0.437 -15.945
He et al. 2022 331.765 50.721 0.75 1.87 -0.44 –

💡 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 – – – – – 98* – –
Cavallo et al. 2024 1.28 0.86 – 302 0.060 – – –
Hunt & Reffert 2023 1.23 0.60 0.61 176 – – – –
He et al. 2022 1.48 0.78 – 79 0.370 – – –

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

Visualization

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