HXHWL 62

Click to load Aladin Lite
0.50 UTI
0.52
CN
1.0
Cdens
0.38
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 5.0 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HXHWL 62 is a moderately populated, very dense object of low 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.
Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 108.142 -20.517 0.509 -1.627 0.69 69.869
Hu & Soubiran 2025 108.142 -20.523 – – – –
Hunt & Reffert 2024 108.158 -20.541 0.514 -1.605 0.68 36.322
Cavallo et al. 2024 108.142 -20.523 0.522 – – –
Hunt & Reffert 2023 108.158 -20.541 0.514 -1.605 0.68 36.322
He et al. 2021 108.146 -20.515 0.49 -1.6 0.67 –

💡 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
Hu & Soubiran 2025 – – – – -0.170* – – –
Hunt & Reffert 2024 – – – – – 222* – –
Cavallo et al. 2024 1.74 1.43 – 603 0.010 – – –
Hunt & Reffert 2023 1.78 1.37 0.90 421 – – – –
He et al. 2021 1.82 1.92 – 240 0.457 – – –

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

Visualization

â„šī¸