HXHWL 68

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0.40 UTI
0.46
CN
0.31
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 14.9 [arcmin]
  • CN 0.46 Poorly 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 68 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
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 – 126.362 -45.47 0.8 -6.303 4.958 5.626
Hunt & Reffert 2024 126.184 -45.438 0.805 -6.287 4.967 8.812
Cavallo et al. 2024 126.322 -45.513 0.808 – – –
Hunt & Reffert 2023 126.184 -45.438 0.805 -6.287 4.967 8.812
He et al. 2021 126.484 -45.582 0.82 -6.29 5.02 –

💡 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
Hunt & Reffert 2024 – – – – – 53* – –
Cavallo et al. 2024 1.29 0.67 – 324 0.330 – – –
Hunt & Reffert 2023 1.17 0.40 0.47 175 – – – –
He et al. 2021 1.15 0.84 – 60 0.112 – – –

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

Visualization

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