CWNU 2417

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0.41 UTI
0.29
CN
0.49
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 2.5 [N/pc2]
  • CN 0.29 Poorly populated
  • Cdens 0.49 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 2417 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, below 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.

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– 236.393 -58.228 0.373 -3.591 -4.293 -62.702
Hunt & Reffert 2024 236.401 -58.241 0.367 -3.576 -4.271 -51.908
Cavallo et al. 2024 236.41 -58.233 0.369 – – –
Hunt & Reffert 2023 236.401 -58.241 0.367 -3.576 -4.271 -51.908
He et al. 2023 236.355 -58.244 0.373 -3.595 -4.287 -62.7

💡 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– 2.4 1.6 0.56 262 0.160 179 – –
Hunt & Reffert 2024 – – – – – 179(1) – –
Cavallo et al. 2024 2.40 1.90 – 234 0.160 – – –
Hunt & Reffert 2023 2.48 1.60 0.56 262 – – – –
He et al. 2023 2.40 1.60 – 708 – – – –

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

Visualization

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