CWNU 3712

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0.46 UTI
0.31
CN
1.0
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
C3 classification AA
Number of members (P>50%) 31
Radius (P>50% members) 0.9 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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CWNU 3712 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.
Very distant High extinction Old

Data
🔍 Search references for CWNU 3712 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 145.542 -54.471 0.154 -4.607 2.771 26.632
He et al. 2023 145.542 -54.473 0.15 -4.61 2.765 26.63

💡 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
He et al. 2023 5.01 3.75 – 1585 – – – –

Visualization
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CWNU 3712 UCC
Galactocentric position diagram