HXHWL 20

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0.57 UTI
0.62
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.9 [arcmin]
  • CN 0.62 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HXHWL 20 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Young

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 – 193.312 -63.75 0.65 -6.307 -1.532 -13.34
Hunt & Reffert 2024 193.288 -63.75 0.646 -6.319 -1.532 -11.561
Cavallo et al. 2024 193.293 -63.733 0.651 – – –
Hunt & Reffert 2023 193.288 -63.75 0.646 -6.319 -1.532 -11.561
He et al. 2021 193.327 -63.723 0.63 -6.34 -1.58 –

💡 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 – – – – – 389* – –
Cavallo et al. 2024 0.94 2.06 – 407 -0.960 – – –
Hunt & Reffert 2023 1.46 1.79 1.69 67 – – – –
He et al. 2021 1.32 2.04 – 87 0.457 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14142 47.9 193.27 -63.73 0.66 -6.35 -1.52 -11.49 0.03

💡 Note: The % column shows the percentage of members that HXHWL 20 shares with each listed object.

Visualization

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