HXHWL 48

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0.53 UTI
0.39
CN
0.89
Cdens
0.75
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 4.5 [N/pc2]
  • CN 0.39 Poorly populated
  • Cdens 0.89 Dense
  • CC3 0.75 High quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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HXHWL 48 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is poorly studied in the literature.

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

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 113.466 -8.233 0.905 -3.54 0.983 16.691
Hu & Soubiran 2025 113.481 -8.245 – – – –
Hunt & Reffert 2024 113.452 -8.261 0.898 -3.535 0.974 7.143
Cavallo et al. 2024 113.481 -8.245 0.912 – – –
Hunt & Reffert 2023 113.452 -8.261 0.898 -3.535 0.974 7.143
He et al. 2021 113.473 -8.264 0.9 -3.59 0.99 –

💡 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] Bfrac BSS
UCC 99999– 1.06 0.21 0.6 321 0.120 110 – –
Hu & Soubiran 2025 – – – – -0.140(5) – – –
Hunt & Reffert 2024 – – – – – 110(1) – –
Cavallo et al. 2024 1.06 0.22 – 724 0.120 – – –
Hunt & Reffert 2023 1.03 0.21 0.60 321 – – – –
He et al. 2021 1.10 0.12 – 95 0.537 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14490 89.7 113.47 -8.23 0.92 -3.53 0.98 14.78 0.0

💡 Note: The % column shows the percentage of members that HXHWL 48 shares with each listed object.

Visualization

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