HXHWL 45

(H21OC 45)

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0.54 UTI
0.56
CN
1.0
Cdens
0.38
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 7.5 [arcmin]
  • CN 0.56 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.38 Low quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

HXHWL 45 is a moderately populated, very dense object of low 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, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.

Data

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 350.356 58.366 1.0 -0.37 -0.916 -21.222
Zhang et al. 2024 350.367 58.367
Hunt & Reffert 2024 350.367 58.367 0.995 -0.322 -0.95 -20.547
Cavallo et al. 2024 350.304 58.357 0.998
Hunt & Reffert 2023 350.367 58.367 0.995 -0.322 -0.95 -20.547
He et al. 2022 350.321 58.363 0.999 -0.37 -0.915
He et al. 2021 350.367 58.381 0.99 -0.42 -0.83

💡 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 -0.124*
Hunt & Reffert 2024 174*
Cavallo et al. 2024 1.04 2.26 68 0.360
Hunt & Reffert 2023 0.96 2.13 0.85 68
He et al. 2022 2.45 50
He et al. 2021 0.95 2.64 79 0.274

💡 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.

Visualization

Galactocentric position diagram

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