CWNU 1436

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0.39 UTI
0.3
CN
0.43
Cdens
0.62
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 2.2 [N/pc2]
  • CN 0.3 Poorly populated
  • Cdens 0.43 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1436 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a significant percentage of members with a later 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– 100.209 13.152 0.258 -0.6 -0.565 60.791
Zhang et al. 2024 100.227 13.162 – – – –
Hunt & Reffert 2024 100.227 13.162 0.274 -0.588 -0.57 60.799
Cavallo et al. 2024 100.211 13.152 0.269 – – –
Hunt & Reffert 2023 100.227 13.162 0.274 -0.588 -0.57 60.799
He et al. 2023 100.195 13.148 0.276 -0.61 -0.602 60.79

💡 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– 3.53 1.4 0.97 141 -0.203 229 – –
Zhang et al. 2024 – – – – -0.275(1) – – –
Hunt & Reffert 2024 – – – – – 229(1) – –
Cavallo et al. 2024 3.24 1.58 – 120 -0.130 – – –
Hunt & Reffert 2023 3.53 0.94 0.97 368 – – – –
He et al. 2023 3.55 1.40 – 141 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 12530 60.0 100.19 13.13 0.28 -0.6 -0.61 – 0.05

💡 Note: The % column shows the percentage of members that CWNU 1436 shares with each listed object.

Visualization

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