HXHWL 59

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0.42 UTI
0.35
CN
0.88
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.1 [arcmin]
  • CN 0.35 Poorly populated
  • Cdens 0.88 Dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HXHWL 59 is a poorly populated, dense object of low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. 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 – 114.955 -18.92 0.422 -2.243 2.218 –
Hunt & Reffert 2024 114.963 -18.912 0.417 -2.253 2.238 –
Cavallo et al. 2024 114.962 -18.939 0.418 – – –
Hunt & Reffert 2023 114.963 -18.912 0.417 -2.253 2.238 –
He et al. 2021 114.947 -18.922 0.41 -2.23 2.19 –

💡 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 – – – – – 212* – –
Cavallo et al. 2024 2.37 1.33 – 76 0.120 – – –
Hunt & Reffert 2023 2.22 1.09 0.58 97 – – – –
He et al. 2021 2.51 1.80 – 33 0.323 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1381 85.7 114.95 -18.92 0.43 -2.24 2.22 – 0.01
CWWDL 13799 71.4 114.95 -18.92 0.44 -2.23 2.22 – 0.01

💡 Note: The % column shows the percentage of members that HXHWL 59 shares with each listed object.

Visualization

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