HXHWL 29

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0.63 UTI
0.64
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 12.6 [arcmin]
  • CN 0.64 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HXHWL 29 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low 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 moderate percentage of members with a later reported entry. See table with shared members information.

Close Low 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 – 268.068 -27.023 1.662 0.882 -5.12 0.191
Hunt & Reffert 2024 268.076 -27.035 1.643 0.9 -5.087 0.744
Cavallo et al. 2024 268.135 -26.938 1.644 – – –
Hunt & Reffert 2023 268.076 -27.035 1.643 0.9 -5.087 0.744
He et al. 2021 268.043 -27.037 1.66 0.89 -5.12 –

💡 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 – – – – – 234* – –
Cavallo et al. 2024 0.55 1.31 – 79 -0.530 – – –
Hunt & Reffert 2023 0.58 0.49 0.85 89 – – – –
He et al. 2021 0.63 0.96 – 50 0.414 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14643 34.6 268.07 -27.04 1.68 0.88 -5.17 -0.84 0.0

💡 Note: The % column shows the percentage of members that HXHWL 29 shares with each listed object.

Visualization

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