CWNU 117

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0.07 UTI
0.3
CN
0.42
Cdens
0.75
CC3
0.25
Clit
0.17
Cdup
Stellar density (N50/rad) 2.1 [N/pc2]
  • CN 0.3 Poorly populated
  • Cdens 0.42 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.17 Likely duplicate

Overview

â„šī¸
CWNU 117 is a poorly 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, 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

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 341.242 57.525 0.639 -3.949 -2.97 -24.995
Hunt & Reffert 2024 341.148 57.53 0.637 -3.947 -2.968 -24.987
Cavallo et al. 2024 341.222 57.498 0.64 – – –
Hunt & Reffert 2023 341.148 57.53 0.637 -3.947 -2.968 -24.987
He et al. 2022 341.204 57.538 0.64 -3.95 -2.97 -26.3

💡 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– 1.52 1.38 0.38 126 -0.241 126 – –
Hunt & Reffert 2024 – – – – – 126(1) – –
Cavallo et al. 2024 1.74 1.39 – 78 0.160 – – –
Hunt & Reffert 2023 1.52 0.94 0.38 155 – – – –
He et al. 2022 1.48 1.38 – 126 -0.642 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0187 83.3 341.22 57.54 0.64 -3.94 -2.97 -24.99 0.28

💡 Note: The % column shows the percentage of members that CWNU 117 shares with each listed object.

Visualization

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