CWNU 1844

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0.28 UTI
0.27
CN
0.28
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.4 [N/pc2]
  • CN 0.27 Poorly populated
  • Cdens 0.28 Loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
CWNU 1844 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young 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)
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– 346.672 59.098 0.263 -3.212 -2.058 –
Hunt & Reffert 2024 346.692 59.099 0.25 -3.223 -2.05 –
Cavallo et al. 2024 346.667 59.103 0.249 – – –
Hunt & Reffert 2023 346.692 59.099 0.25 -3.223 -2.05 –
He et al. 2023 346.682 59.101 0.26 -3.208 -2.043 –

💡 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– 3.8 3.37 0.66 15 0.290 361 – –
Hunt & Reffert 2024 – – – – – 361(1) – –
Cavallo et al. 2024 2.61 2.90 – 166 0.290 – – –
Hunt & Reffert 2023 3.96 3.37 0.66 15 – – – –
He et al. 2023 3.80 3.65 – 7 – – – –

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

Visualization

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