CWNU 2471

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0.24 UTI
0.54
CN
0.11
Cdens
0.75
CC3
0.31
Clit
0.6
Cdup
Radius (P>50% members) 8.7 [arcmin]
  • CN 0.54 Moderately populated
  • Cdens 0.11 Very loose
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 0.6 Likely unique

Overview

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CWNU 2471 is a moderately populated, very loose object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Distant Moderate extinction Near-solar metallicity Young

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 92.571 12.899 0.251 -0.491 -0.646 –
Zhang et al. 2024 92.558 12.831 – – – –
Hunt & Reffert 2024 92.558 12.831 0.253 -0.484 -0.664 –
Cavallo et al. 2024 92.598 12.941 0.256 – – –
Hunt & Reffert 2023 92.558 12.831 0.253 -0.484 -0.664 –
He et al. 2023 92.583 12.962 0.272 -0.492 -0.645 2.26

💡 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 – – – – -0.388* – – –
Hunt & Reffert 2024 – – – – – 487* – –
Cavallo et al. 2024 3.10 1.53 – 186 0.420 – – –
Hunt & Reffert 2023 3.44 1.89 2.08 56 – – – –
He et al. 2023 3.31 2.20 – 28 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0952 39.7 92.55 13.05 0.24 -0.52 -0.63 – 0.32

💡 Note: The % column shows the percentage of members that CWNU 2471 shares with each listed object.

Visualization

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