CWNU 1148

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0.31 UTI
0.35
CN
0.7
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 10.5 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 0.7 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

CWNU 1148 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Moderate extinction Young

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 315.039 38.992 0.963 -3.275 -8.957 -14.924
He et al. 2022 315.044 39.0 0.962 -3.271 -8.947

💡 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
He et al. 2022 1.25 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.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 3916 100.0 315.1 38.99 0.96 -3.28 -8.96 -15.5 0.2

💡 Note: The % column shows the percentage of members that CWNU 1148 shares with each listed object.

Visualization

Galactocentric position diagram

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