HXHWL 36

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0.27 UTI
0.25
CN
0.33
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 1.6 [N/pc2]
  • CN 0.25 Poorly populated
  • Cdens 0.33 Loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HXHWL 36 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

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 99999– 123.846 -47.271 0.954 -5.599 5.137 35.845
Hunt & Reffert 2024 123.78 -47.275 0.958 -5.614 5.171 29.237
Cavallo et al. 2024 123.88 -47.255 0.963 – – –
Hunt & Reffert 2023 123.78 -47.275 0.958 -5.614 5.171 29.237
He et al. 2021 123.912 -47.235 0.93 -5.61 5.11 –

💡 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] Bfrac BSS
UCC 99999– 1.0 0.39 0.35 98 0.297 59 – –
Hunt & Reffert 2024 – – – – – 59(1) – –
Cavallo et al. 2024 1.00 0.39 – 141 0.020 – – –
Hunt & Reffert 2023 1.00 0.14 0.35 98 – – – –
He et al. 2021 1.05 0.48 – 76 0.575 – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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