CWNU 1843

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0.32 UTI
0.29
CN
0.56
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.8 [N/pc2]
  • CN 0.29 Poorly populated
  • Cdens 0.56 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 1843 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, intermediate-age 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 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– 149.358 -55.573 0.459 -6.466 3.318 –
Hunt & Reffert 2024 149.459 -55.565 0.451 -6.461 3.347 –
Cavallo et al. 2024 149.325 -55.553 0.453 – – –
Hunt & Reffert 2023 149.459 -55.565 0.451 -6.461 3.347 –
He et al. 2023 149.331 -55.535 0.476 -6.465 3.32 –

💡 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– 2.0 1.9 0.92 139 -0.580 233 – –
Hunt & Reffert 2024 – – – – – 233(1) – –
Cavallo et al. 2024 1.96 2.31 – 275 -0.580 – – –
Hunt & Reffert 2023 2.10 1.69 0.92 139 – – – –
He et al. 2023 2.00 1.90 – 32 – – – –

(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 13562 69.0 149.35 -55.54 0.46 -6.41 3.36 12.43 0.09

💡 Note: The % column shows the percentage of members that CWNU 1843 shares with each listed object.

Visualization

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