CWNU 427

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0.47 UTI
0.52
CN
0.45
Cdens
0.75
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 13.4 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 0.45 Loose
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 427 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near 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)
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 – 302.645 30.641 0.796 -0.26 -3.101 -1.146
Zhang et al. 2024 302.722 30.633 – – – –
Hunt & Reffert 2024 302.722 30.633 0.786 -0.234 -3.081 1.514
Cavallo et al. 2024 302.591 30.646 0.789 – – –
Hunt & Reffert 2023 302.722 30.633 0.786 -0.234 -3.081 1.514
He et al. 2022 302.565 30.562 0.78 -0.25 -3.1 –

💡 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
Zhang et al. 2024 – – – – -0.046* – – –
Hunt & Reffert 2024 – – – – – 128* – –
Cavallo et al. 2024 1.24 1.65 – 59 -0.020 – – –
Hunt & Reffert 2023 1.20 1.23 0.43 126 – – – –
He et al. 2022 1.74 2.04 – 25 -0.236 – – –

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

Visualization

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