CWNU 1546

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0.34 UTI
0.38
CN
0.34
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.7 [N/pc2]
  • CN 0.38 Poorly populated
  • Cdens 0.34 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1546 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a large distance, above 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 age parameter (see Parameters). It was recently reported in the literature.

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 99999– 340.721 64.088 0.172 -2.147 -1.104 -98.237
Hunt & Reffert 2024 340.746 64.12 0.168 -2.17 -1.108 -105.352
Cavallo et al. 2024 340.691 64.099 0.169 – – –
Hunt & Reffert 2023 340.746 64.12 0.168 -2.17 -1.108 -105.352
He et al. 2023 340.697 64.062 0.206 -2.132 -1.125 -96.08

💡 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– 5.62 2.8 1.78 306 0.250 836 – –
Hunt & Reffert 2024 – – – – – 836(1) – –
Cavallo et al. 2024 10.57 2.67 – 224 0.250 – – –
Hunt & Reffert 2023 5.62 2.84 1.78 306 – – – –
He et al. 2023 5.62 2.80 – 794 – – – –

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

Visualization

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