HXHWL 65

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0.54 UTI
0.35
CN
1.0
Cdens
0.75
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 5.7 [N/pc2]
  • CN 0.35 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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HXHWL 65 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a 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 absorption parameter (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.

Liu et al. (2025)
Classified as tidal capture (resonant trapping binary) 259 along with Ruprecht_53.

Palma et al. (2025)
Classified as optical pair P538, along with Ruprecht_53.

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– 122.413 -27.151 1.006 -3.955 2.026 8.093
Hunt & Reffert 2024 122.424 -27.136 0.992 -3.942 2.038 7.18
Cavallo et al. 2024 122.409 -27.131 0.997 – – –
Hunt & Reffert 2023 122.424 -27.136 0.992 -3.942 2.038 7.18
He et al. 2021 122.377 -27.159 0.99 -3.93 2.0 –

💡 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– 1.025 0.105 0.19 288 0.485 77 – –
Liu et al. 2025 1.24 0.13 – 204 – – – –
Hunt & Reffert 2024 – – – – – 77(1) – –
Cavallo et al. 2024 1.00 0.00 – 372 0.360 – – –
Hunt & Reffert 2023 0.92 0.08 0.19 478 – – – –
He et al. 2021 1.05 0.24 – 158 0.611 – – –

(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 14423 94.3 122.41 -27.15 1.01 -3.96 2.03 8.57 0.01

💡 Note: The % column shows the percentage of members that HXHWL 65 shares with each listed object.

Visualization

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