CWNU 10

Click to load Aladin Lite
0.07 UTI
0.26
CN
0.55
Cdens
0.38
CC3
0.31
Clit
0.19
Cdup
Radius (P>50% members) 10.7 [arcmin]
  • CN 0.26 Poorly populated
  • Cdens 0.55 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 0.19 Likely duplicate

Overview

CWNU 10 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a close distance, above the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously 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 95.286 18.841 1.011 -1.801 -2.851 -10.86
Zhang et al. 2024 95.318 18.827
Hunt & Reffert 2024 95.318 18.827 0.989 -1.763 -2.849 0.035
Cavallo et al. 2024 95.254 18.896 0.987
Hunt & Reffert 2023 95.318 18.827 0.989 -1.763 -2.849 0.035
He et al. 2022 95.281 18.871 1.01 -1.74 -2.85

💡 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
Zhang et al. 2024 -0.237*
Hunt & Reffert 2024 131*
Cavallo et al. 2024 1.07 0.88 186 0.250
Hunt & Reffert 2023 0.95 0.79 1.69 286
He et al. 2022 1.17 0.78 251 0.968

💡 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.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
LP 34 80.8 95.31 18.83 1.02 -1.81 -2.85 -10.3 0.28

💡 Note: The % column shows the percentage of members that CWNU 10 shares with each listed object.

Visualization

Galactocentric position diagram

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