CWNU 346

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0.26 UTI
0.26
CN
1.0
Cdens
0.62
CC3
0.0
Clit
0.69
Cdup
Stellar density (N50/rad) 8.3 [N/pc2]
  • CN 0.26 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.69 Likely unique

Overview

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CWNU 346 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is rarely studied in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Palma et al. (2025)
Classified as optical pair P369, along with HSC_1086.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 34.522 61.154 0.477 -0.82 -0.24 -59.52
Hunt & Reffert 2024 34.546 61.156 0.487 -0.832 -0.245 -59.511
Hunt & Reffert 2023 34.546 61.156 0.487 -0.832 -0.245 -59.511
He et al. 2022 34.502 61.153 0.46 -0.84 -0.25 -61.2

💡 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– 1.905 4.015 1.01 41 0.968 406 – –
Hunt & Reffert 2024 – – – – – 406(1) – –
Hunt & Reffert 2023 2.11 4.25 1.01 3 – – – –
He et al. 2022 1.70 3.78 – 79 0.968 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0578 30.8 34.99 61.03 0.44 -1.11 -0.29 -65.66 0.29

💡 Note: The % column shows the percentage of members that CWNU 346 shares with each listed object.

Visualization

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