CWNU 1183

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0.36 UTI
0.25
CN
0.32
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 28.5 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.32 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

CWNU 1183 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a very close distance, above the mid-plane. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a moderate percentage of members with at least one entry reported in the same catalogue. 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 295.927 38.469 2.088 1.422 -0.83 -10.271
Zhang et al. 2024 295.611 38.272
Cavallo et al. 2024 297.33 39.789 2.075
Hunt & Reffert 2023 295.611 38.272 2.07 1.491 -0.592 -7.079
He et al. 2022 295.669 38.276 2.107 1.325 -1.214

💡 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 -0.070*
Cavallo et al. 2024 0.52 0.64 21 0.070
Hunt & Reffert 2023 0.46 0.11 0.59 46
He et al. 2022 0.10 45

💡 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
Theia 540 36.0 296.62 39.82 2.11 1.47 -0.65 -9.9 0.16

💡 Note: The % column shows the percentage of members that CWNU 1183 shares with each listed object.

Visualization

Galactocentric position diagram

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