CWNU 1726

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0.39 UTI
0.34
CN
0.59
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.9 [arcmin]
  • CN 0.34 Poorly populated
  • Cdens 0.59 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

CWNU 1726 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 233.08 -58.589 0.421 -3.218 -4.356 -42.309
Hunt & Reffert 2024 233.077 -58.596 0.409 -3.205 -4.371 12.409
Cavallo et al. 2024 233.1 -58.577 0.409
Hunt & Reffert 2023 233.077 -58.596 0.409 -3.205 -4.371 12.409
He et al. 2023 233.089 -58.595 0.422 -3.225 -4.354 -42.31

💡 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 377*
Cavallo et al. 2024 2.39 2.18 135 0.370
Hunt & Reffert 2023 2.26 1.95 1.22 249
He et al. 2023 2.24 2.20 398

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

Visualization

Galactocentric position diagram

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