HXHWL 30

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0.54 UTI
0.54
CN
0.91
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.5 [N/pc2]
  • CN 0.54 Moderately populated
  • Cdens 0.91 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HXHWL 30 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate 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 significant 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– 284.63 -9.97 0.928 1.187 0.801 -1.303
Hunt & Reffert 2024 284.683 -9.862 0.912 1.177 0.795 -1.988
Cavallo et al. 2024 284.607 -9.939 0.915 – – –
Hunt & Reffert 2023 284.683 -9.862 0.912 1.177 0.795 -1.988
He et al. 2021 284.641 -9.962 0.94 1.13 0.84 –

💡 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– 1.09 1.32 0.36 204 0.218 172 – –
Hunt & Reffert 2024 – – – – – 172(1) – –
Cavallo et al. 2024 1.09 1.32 – 162 -0.100 – – –
Hunt & Reffert 2023 1.03 0.85 0.36 204 – – – –
He et al. 2021 1.15 1.32 – 316 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 14332 72.4 284.63 -9.97 0.93 1.16 0.81 -3.48 0.0

💡 Note: The % column shows the percentage of members that HXHWL 30 shares with each listed object.

Visualization

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