HXHWL 72

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0.29 UTI
0.0
CN
0.18
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 10.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.18 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HXHWL 72 is a sparse, very loose object of high C3 quality. Its parallax locates it at a relatively close distance, near 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 – 105.297 -3.816 0.592 -0.138 -0.791 12.79
Hunt & Reffert 2024 105.296 -3.738 0.56 -0.118 -0.777 32.032
Cavallo et al. 2024 105.325 -3.961 0.56 – – –
Hunt & Reffert 2023 105.296 -3.738 0.56 -0.118 -0.777 32.032
He et al. 2021 105.377 -3.865 0.64 -0.15 -0.8 –

💡 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 – – – – – 93* – –
Cavallo et al. 2024 1.77 0.35 – 417 0.240 – – –
Hunt & Reffert 2023 1.63 0.17 0.79 494 – – – –
He et al. 2021 1.82 0.60 – 72 0.611 – – –

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

Visualization

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