CWNU 1381

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0.25 UTI
0.41
CN
0.72
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 5.0 [arcmin]
  • CN 0.41 Poorly populated
  • Cdens 0.72 Moderately dense
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

CWNU 1381 is a poorly populated, moderately dense object of very low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane. It is catalogued as an intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 61.691 48.87 0.431 0.393 -0.986 -48.044
He et al. 2023 61.691 48.868 0.441 0.373 -0.987

💡 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 2.04 2.25 355

💡 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
Theia 2493 82.9 61.69 48.86 0.42 0.39 -0.98 -48.04 0.02

💡 Note: The % column shows the percentage of members that CWNU 1381 shares with each listed object.

Visualization

Galactocentric position diagram

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