CWNU 348

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0.55 UTI
0.49
CN
1.0
Cdens
0.62
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.49 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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CWNU 348 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate 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 is poorly studied in the literature.
Relatively close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Wood sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 328.11 64.939 0.897 -2.124 -4.561 -27.998
Hunt & Reffert 2024 328.135 64.946 0.917 -2.097 -4.572 -11.014
Cavallo et al. 2024 328.119 64.966 0.902 – – –
Hunt & Reffert 2023 328.135 64.946 0.917 -2.097 -4.572 -11.014
He et al. 2022 328.117 64.96 0.889 -2.135 -4.579 –
He et al. 2022 328.125 64.967 0.89 -2.13 -4.56 -10.6

💡 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 – – – – – 89* – –
Cavallo et al. 2024 1.15 1.27 – 48 0.370 – – –
Hunt & Reffert 2023 1.10 1.46 2.31 6 – – – –
He et al. 2022 – 1.35 – 2 – – – –
He et al. 2022 0.83 1.08 – 4 -0.642 – – –

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

Visualization

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