HXWHB 10

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0.37 UTI
0.25
CN
0.6
Cdens
0.38
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.6 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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HXWHB 10 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, near 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 metallicity 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.

Relatively close Low extinction Near-solar metallicity Intermediate age

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 – 81.904 33.285 0.382 1.289 -2.858 18.467
Zhang et al. 2024 81.93 33.283 – – – –
Hunt & Reffert 2024 81.93 33.283 0.387 1.258 -2.836 5.788
Cavallo et al. 2024 81.908 33.283 0.387 – – –
Hunt & Reffert 2023 81.93 33.283 0.387 1.258 -2.836 5.788
Hao et al. 2020 81.94 33.28 0.32 1.32 -2.93 –

💡 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
Zhang et al. 2024 – – – – -0.334* – – –
Hunt & Reffert 2024 – – – – – 343* – –
Cavallo et al. 2024 2.32 0.80 – 490 0.380 – – –
Hunt & Reffert 2023 2.27 0.94 0.72 404 – – – –
Hao et al. 2020 3.09 1.54 – 316 – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1283 100.0 81.9 33.3 0.39 1.29 -2.85 18.47 0.13

💡 Note: The % column shows the percentage of members that HXWHB 10 shares with each listed object.

Visualization

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