HXHWL 49

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0.49 UTI
0.42
CN
0.79
Cdens
0.62
CC3
0.3
Clit
1.0
Cdup
Stellar density (N50/rad) 3.9 [N/pc2]
  • CN 0.42 Poorly populated
  • Cdens 0.79 Dense
  • CC3 0.62 Intermediate quality
  • Clit 0.3 Poorly studied
  • Cdup 1.0 Unique

Overview

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HXHWL 49 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (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.

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– 77.707 36.371 0.641 1.108 -4.011 -6.011
Zhang et al. 2024 77.703 36.365 – – – –
Hunt & Reffert 2024 77.703 36.365 0.644 1.118 -4.02 -5.958
Cavallo et al. 2024 77.731 36.363 0.642 – – –
Hunt & Reffert 2023 77.703 36.365 0.644 1.118 -4.02 -5.958
He et al. 2021 77.708 36.357 0.6 1.15 -3.97 –

💡 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– 1.51 1.26 0.82 120 0.350 161 – –
Zhang et al. 2024 – – – – -0.215(1) – – –
Hunt & Reffert 2024 – – – – – 161(1) – –
Cavallo et al. 2024 1.57 1.26 – 98 0.350 – – –
Hunt & Reffert 2023 1.46 1.04 0.82 120 – – – –
He et al. 2021 1.51 1.44 – 151 0.457 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 1277 76.2 77.71 36.38 0.64 1.1 -4.05 -6.01 0.0

💡 Note: The % column shows the percentage of members that HXHWL 49 shares with each listed object.

Visualization

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