CWNU 1053

(OCSN 169)

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0.47 UTI
0.58
CN
0.52
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 34.2 [arcmin]
  • CN 0.58 Moderately populated
  • Cdens 0.52 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

CWNU 1053 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane. It is catalogued as a near-solar metallicity, intermediate-age 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 163.207 -56.513 1.973 -17.816 6.37 -2.001
Cavallo et al. 2024 162.374 -56.558 1.892
Hunt & Reffert 2023 162.419 -56.608 1.876 -17.213 6.219 -2.459
Qin et al. 2023 163.16 -56.45 1.99 -17.99 6.31 -2.1
He et al. 2022 163.481 -56.316 2.007 -18.058 6.288

💡 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
Cavallo et al. 2024 0.54 0.29 204 0.250
Hunt & Reffert 2023 0.51 0.15 0.75 151
Qin et al. 2023 0.61 0.40 89
He et al. 2022 0.45 79

💡 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.

Visualization

Galactocentric position diagram

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