CWNU 501

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0.50 UTI
0.27
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 7.1 [arcmin]
  • CN 0.27 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 501 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 102.043 -16.901 0.969 -3.508 5.115 30.724
Hunt & Reffert 2024 102.102 -16.883 0.944 -3.547 5.154 23.141
Cavallo et al. 2024 101.984 -16.899 0.954 – – –
Hunt & Reffert 2023 102.102 -16.883 0.944 -3.547 5.154 23.141
He et al. 2022 102.082 -16.9 0.97 -3.5 5.12 60.4

💡 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 – – – – – 74* – –
Cavallo et al. 2024 1.32 1.33 – 24 -0.130 – – –
Hunt & Reffert 2023 1.00 1.18 1.96 18 – – – –
He et al. 2022 0.85 1.14 – 32 0.457 – – –

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

Visualization

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