HXHWL 43

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0.27 UTI
0.38
CN
0.49
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 9.1 [arcmin]
  • CN 0.38 Poorly populated
  • Cdens 0.49 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

HXHWL 43 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. It is catalogued as a metal-rich, intermediate-age cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a significant percentage of members with 2 later reported entries. 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 115.479 -21.846 0.669 -2.5 1.692 40.047
He et al. 2021 115.476 -21.804 0.66 -2.52 1.65

💡 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. 2021 1.51 0.36 288 0.537

💡 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
CWWDL 14179 65.8 115.54 -21.87 0.68 -2.51 1.71 39.8 0.03
Theia 3524 50.0 115.55 -21.98 0.68 -2.5 1.72 34.46 0.05

💡 Note: The % column shows the percentage of members that HXHWL 43 shares with each listed object.

Visualization

Galactocentric position diagram

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