CWNU 1074

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0.36 UTI
0.0
CN
0.81
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 10.8 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.81 Dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

CWNU 1074 is a sparse, dense object of intermediate C3 quality. Its parallax locates it at a close distance, below the mid-plane. It is catalogued as a near-solar metallicity, 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 295.836 6.335 1.347 0.545 -2.003 -8.005
Hunt & Reffert 2024 295.903 6.413 1.338 0.355 -2.036 -8.561
Cavallo et al. 2024 295.442 5.261 1.343
Hunt & Reffert 2023 295.903 6.413 1.338 0.355 -2.036 -8.561
He et al. 2022 295.892 6.445 1.334 0.574 -1.961

💡 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 99*
Cavallo et al. 2024 0.76 0.77 29 -0.040
Hunt & Reffert 2023 0.71 0.64 0.80 36
He et al. 2022 0.90 35

💡 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.