CWNU 73

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0.52 UTI
0.35
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 5.2 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 73 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above 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 – 168.085 -57.922 0.723 -9.071 1.806 -27.846
Hunt & Reffert 2024 168.088 -57.942 0.713 -9.059 1.826 -38.45
Cavallo et al. 2024 168.105 -57.912 0.72 – – –
Hunt & Reffert 2023 168.088 -57.942 0.713 -9.059 1.826 -38.45
He et al. 2022 168.096 -57.911 0.74 -9.07 1.8 –

💡 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 – – – – – 147* – –
Cavallo et al. 2024 1.27 0.38 – 295 -0.170 – – –
Hunt & Reffert 2023 1.33 0.15 0.51 137 – – – –
He et al. 2022 1.15 0.48 – 63 -0.642 – – –

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

Visualization

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