CWNU 1582

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0.43 UTI
0.29
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 10.6 [N/pc2]
  • CN 0.29 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1582 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It was recently reported in the literature.

Note: This object shares a small 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– 314.308 44.82 0.176 -2.9 -3.798 –
Hunt & Reffert 2024 314.302 44.82 0.174 -2.902 -3.806 –
Cavallo et al. 2024 314.304 44.823 0.173 – – –
Hunt & Reffert 2023 314.302 44.82 0.174 -2.902 -3.806 –
He et al. 2023 314.301 44.824 0.176 -2.9 -3.798 –

💡 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– 5.18 4.05 2.17 22 0.200 1025 – –
Hunt & Reffert 2024 – – – – – 1025(1) – –
Cavallo et al. 2024 5.40 4.05 – 22 0.200 – – –
Hunt & Reffert 2023 5.18 3.71 2.17 156 – – – –
He et al. 2023 4.47 4.15 – 16 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CKCWDM 44145 10.3 314.47 44.94 0.16 -2.67 -3.81 -31.12 0.03

💡 Note: The % column shows the percentage of members that CWNU 1582 shares with each listed object.

Visualization

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