CWNU 3449

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0.31 UTI
0.0
CN
0.55
Cdens
1.0
CC3
0.0
Clit
1.0
Cdup
C3 classification AA
Number of members (P>50%) 23
Radius (P>50% members) 1.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.55 Moderately 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 3449 is a sparse, moderately dense object of very high C3 quality. Its parallax locates it at a large distance, well below the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It was recently reported in the literature.
Very distant Low extinction Old

Data
🔍 Search references for CWNU 3449 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 – 93.887 2.221 0.141 -0.198 -0.131 73.713
He et al. 2023 93.889 2.214 0.135 -0.213 -0.112 82.8

💡 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 7.08 1.00 – 1585 – – – –

Visualization
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CWNU 3449 UCC
Galactocentric position diagram