CWNU 368

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0.43 UTI
0.29
CN
1.0
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • 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 368 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Intermediate age

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 – 69.962 50.305 0.376 0.157 0.088 -38.404
Hunt & Reffert 2024 69.941 50.298 0.374 0.168 0.09 -38.404
Cavallo et al. 2024 69.958 50.307 0.373 – – –
Hunt & Reffert 2023 69.941 50.298 0.374 0.168 0.09 -38.404
He et al. 2022 69.959 50.306 0.39 0.11 0.09 -38.4

💡 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] Bfr BSS
Hunt & Reffert 2024 – – – – – 364* – –
Cavallo et al. 2024 2.39 2.89 – 234 -0.240 – – –
Hunt & Reffert 2023 2.39 2.80 1.90 160 – – – –
He et al. 2022 2.00 2.88 – 316 -0.236 – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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