HXHWL 8

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0.42 UTI
0.56
CN
0.31
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.5 [N/pc2]
  • CN 0.56 Moderately populated
  • Cdens 0.31 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HXHWL 8 is a moderately populated, loose 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 (see Parameters). It is poorly studied in the literature.

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– 319.227 44.012 0.843 0.065 -4.388 -12.345
Hunt & Reffert 2024 319.224 44.084 0.835 0.06 -4.376 -11.512
Cavallo et al. 2024 319.344 44.038 0.837 – – –
Hunt & Reffert 2023 319.224 44.084 0.835 0.06 -4.376 -11.512
He et al. 2021 319.334 43.978 0.85 0.05 -4.35 –

💡 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– 1.14 1.13 1.0 195 0.477 161 – –
Hunt & Reffert 2024 – – – – – 161(1) – –
Cavallo et al. 2024 1.11 1.13 – 195 0.380 – – –
Hunt & Reffert 2023 1.14 1.13 1.00 128 – – – –
He et al. 2021 1.20 1.20 – 347 0.575 – – –

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

Visualization

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