HXHWL 17

(H21OC 17)

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0.42 UTI
0.5
CN
0.74
Cdens
0.25
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 11.5 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 0.74 Moderately dense
  • CC3 0.25 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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HXHWL 17 is a moderately populated, moderately dense object of low 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.

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

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 – 109.276 -11.986 0.91 -2.109 -0.12 43.408
Hunt & Reffert 2024 109.277 -12.029 0.893 -2.104 -0.09 38.5
Cavallo et al. 2024 109.291 -12.049 0.895 – – –
Hunt & Reffert 2023 109.277 -12.029 0.893 -2.104 -0.09 38.5
He et al. 2022 109.288 -12.036 0.924 -2.069 -0.142 –
He et al. 2021 109.309 -12.044 0.93 -2.11 -0.18 –

💡 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 – – – – – 102* – –
Cavallo et al. 2024 1.06 0.52 – 316 0.200 – – –
Hunt & Reffert 2023 1.05 0.41 0.48 296 – – – –
He et al. 2022 – 0.85 – 282 – – – –
He et al. 2021 1.15 0.84 – 263 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 14381 54.0 109.3 -12.01 0.91 -2.09 -0.12 43.41 0.0

💡 Note: The % column shows the percentage of members that HXHWL 17 shares with each listed object.

Visualization

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