HXHWL 51

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0.61 UTI
0.57
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.6 [arcmin]
  • CN 0.57 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

HXHWL 51 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane. 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 a later reported entry. See table with shared members information.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 278.672 -13.019 0.586 0.654 -0.174 11.746
Hunt & Reffert 2024 278.662 -13.031 0.587 0.64 -0.188
Cavallo et al. 2024 278.678 -13.015 0.587
Hunt & Reffert 2023 278.662 -13.031 0.587 0.64 -0.188
He et al. 2021 278.659 -13.02 0.56 0.67 -0.14

💡 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 371*
Cavallo et al. 2024 1.73 1.91 40 0.300
Hunt & Reffert 2023 1.62 1.65 0.63 68
He et al. 2021 1.51 2.28 126 0.498

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1023 87.5 278.68 -13.03 0.59 0.65 -0.17 1.56 0.02

💡 Note: The % column shows the percentage of members that HXHWL 51 shares with each listed object.

Visualization

Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.