HXHWL 13

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0.59 UTI
0.68
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 12.3 [arcmin]
  • CN 0.68 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

HXHWL 13 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above 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 moderate 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

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 218.099 -58.707 0.879 -1.217 -3.079 4.963
Hunt & Reffert 2024 217.999 -58.737 0.873 -1.203 -3.076 -4.459
Cavallo et al. 2024 218.356 -58.657 0.874
Hunt & Reffert 2023 217.999 -58.737 0.873 -1.203 -3.076 -4.459
He et al. 2021 217.995 -58.731 0.87 -1.2 -3.11

💡 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
Hunt & Reffert 2024 204*
Cavallo et al. 2024 1.03 0.99 158 -0.080
Hunt & Reffert 2023 1.08 0.81 0.58 120
He et al. 2021 1.15 1.32 35 0.112

💡 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
CWWDL 14426 42.5 218.02 -58.75 0.88 -1.22 -3.04 8.44 0.0

💡 Note: The % column shows the percentage of members that HXHWL 13 shares with each listed object.

Visualization

Galactocentric position diagram

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