CWNU 385

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0.38 UTI
0.27
CN
0.75
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.3 [arcmin]
  • CN 0.27 Poorly populated
  • Cdens 0.75 Dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 385 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Relatively close Low 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 – 95.497 9.646 0.465 -0.732 -1.162 –
Hunt & Reffert 2024 95.5 9.643 0.452 -0.731 -1.212 –
Cavallo et al. 2024 95.496 9.687 0.451 – – –
Hunt & Reffert 2023 95.5 9.643 0.452 -0.731 -1.212 –
He et al. 2022 95.466 9.675 0.45 -0.71 -1.15 33.1

💡 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 – – – – – 112* – –
Cavallo et al. 2024 2.10 0.88 – 81 0.010 – – –
Hunt & Reffert 2023 2.07 0.65 0.28 205 – – – –
He et al. 2022 2.04 0.48 – 251 0.968 – – –

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

Visualization

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