CWNU 165

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0.43 UTI
0.0
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

CWNU 165 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane. It is catalogued as a metal-poor, young cluster (see Parameters). It is poorly studied in the literature.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 290.088 4.326 0.686 0.112 -0.769 27.52
Hunt & Reffert 2024 290.082 4.33 0.679 0.047 -0.852 12.683
Cavallo et al. 2024 290.075 4.33 0.679
Hunt & Reffert 2023 290.082 4.33 0.679 0.047 -0.852 12.683
He et al. 2022 290.076 4.313 0.7 0.1 -0.77

💡 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 160*
Cavallo et al. 2024 1.61 2.32 69 0.610
Hunt & Reffert 2023 1.42 1.76 1.03 165
He et al. 2022 2.04 1.26 3 -2.028

💡 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.