CWNU 10

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0.07 UTI
0.26
CN
0.55
Cdens
0.38
CC3
0.3
Clit
0.19
Cdup
Stellar density (N50/rad) 2.7 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 0.55 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.3 Poorly studied
  • Cdup 0.19 Likely duplicate

Overview

â„šī¸
CWNU 10 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

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 99999– 95.286 18.841 1.011 -1.801 -2.851 -10.86
Zhang et al. 2024 95.318 18.827 – – – –
Hunt & Reffert 2024 95.318 18.827 0.989 -1.763 -2.849 0.035
Cavallo et al. 2024 95.254 18.896 0.987 – – –
Hunt & Reffert 2023 95.318 18.827 0.989 -1.763 -2.849 0.035
He et al. 2022 95.281 18.871 1.01 -1.74 -2.85 –

💡 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] Bfrac BSS
UCC 99999– 1.07 0.79 1.69 251 0.250 131 – –
Zhang et al. 2024 – – – – -0.237(1) – – –
Hunt & Reffert 2024 – – – – – 131(1) – –
Cavallo et al. 2024 1.07 0.88 – 186 0.250 – – –
Hunt & Reffert 2023 0.95 0.79 1.69 286 – – – –
He et al. 2022 1.17 0.78 – 251 0.968 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
LP 34 80.8 95.31 18.83 1.02 -1.81 -2.85 -10.3 0.28

💡 Note: The % column shows the percentage of members that CWNU 10 shares with each listed object.

Visualization

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