HXHWL 74

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0.51 UTI
0.53
CN
1.0
Cdens
0.38
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 3.0 [arcmin]
  • CN 0.53 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

HXHWL 74 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a moderate 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.

Note: This object shares a significant percentage of members with a later reported entry. 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 103.855 -3.777 0.418 -1.802 1.126 71.289
Hu & Soubiran 2025 103.854 -3.78
Hunt & Reffert 2024 103.861 -3.777 0.423 -1.787 1.14 71.29
Cavallo et al. 2024 103.854 -3.78 0.423
Hunt & Reffert 2023 103.861 -3.777 0.423 -1.787 1.14 71.29
He et al. 2021 103.864 -3.787 0.42 -1.81 1.07

💡 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
Hu & Soubiran 2025 -0.300*
Hunt & Reffert 2024 244*
Cavallo et al. 2024 1.99 1.51 741 -0.220
Hunt & Reffert 2023 2.17 1.13 0.66 427
He et al. 2021 2.09 1.44 575 -0.419

💡 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
UBC 1349 58.9 103.85 -3.78 0.43 -1.81 1.12 71.29 0.0

💡 Note: The % column shows the percentage of members that HXHWL 74 shares with each listed object.

Visualization

Galactocentric position diagram

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