CWWDL 14426

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0.00 UTI
0.37
CN
0.67
Cdens
0.75
CC3
0.0
Clit
0.0
Cdup
C3 classification AB
Number of members (P>50%) 37
Radius (P>50% members) 10.0 [arcmin]
  • CN 0.37 Poorly populated
  • Cdens 0.67 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate
📥 Members 📊 Colab 🔬 Bayestar19 🔍 SciX 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview
CWWDL 14426 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane. It is catalogued as a metal-poor, young cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Metal-poor Young

Data
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 218.02 -58.746 0.876 -1.223 -3.041 8.435
Chi et al. 2023 218.098 -58.748 0.887 -1.193 -3.011 2.911

💡 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
Chi et al. 2023 – – – 41 -0.880 – – –

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
HXHWL 13 100.0 218.1 -58.71 0.88 -1.22 -3.08 4.96 0.59

💡 Note: The % column shows the percentage of members that CWWDL 14426 shares with each listed object.

Visualization
CWWDL 14426 UCC
Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.