HXHWL 35

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0.43 UTI
0.32
CN
0.6
Cdens
0.62
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 5.5 [arcmin]
  • CN 0.32 Poorly populated
  • Cdens 0.6 Moderately dense
  • CC3 0.62 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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HXHWL 35 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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 Moderate 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 – 71.989 44.01 0.491 1.409 -2.16 –
Zhang et al. 2024 72.014 43.967 – – – –
Hunt & Reffert 2024 72.014 43.967 0.492 1.394 -2.164 –
Cavallo et al. 2024 71.965 44.022 0.496 – – –
Hunt & Reffert 2023 72.014 43.967 0.492 1.394 -2.164 –
He et al. 2021 72.022 44.0 0.52 1.43 -2.11 –

💡 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
Zhang et al. 2024 – – – – -0.150* – – –
Hunt & Reffert 2024 – – – – – 217* – –
Cavallo et al. 2024 2.02 1.09 – 54 0.220 – – –
Hunt & Reffert 2023 1.88 1.02 0.48 109 – – – –
He et al. 2021 2.00 1.20 – 275 0.457 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1266 75.0 71.99 44.02 0.49 1.39 -2.17 – 0.01

💡 Note: The % column shows the percentage of members that HXHWL 35 shares with each listed object.

Visualization

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