HSC 1892

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0.35 UTI
0.33
CN
0.56
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.6 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 0.56 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1892 is a poorly populated, moderately dense object of low C3 quality. Its parallax locates it at a moderate distance, below 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 was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Distant Moderate extinction Near-solar metallicity Intermediate age

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 – 110.611 -23.621 0.221 -1.99 2.458 105.692
Hu & Soubiran 2025 110.624 -23.627 – – – –
Hunt & Reffert 2024 110.633 -23.627 0.219 -1.986 2.458 105.663
Cavallo et al. 2024 110.624 -23.627 0.222 – – –
Hunt & Reffert 2023 110.633 -23.627 0.219 -1.986 2.458 105.663

💡 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
Hu & Soubiran 2025 – – – – -0.260* – – –
Hunt & Reffert 2024 – – – – – 331* – –
Cavallo et al. 2024 3.25 2.25 – 1288 0.270 – – –
Hunt & Reffert 2023 3.95 2.24 1.84 467 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2958 93.9 110.61 -23.62 0.22 -1.99 2.48 105.69 0.02

💡 Note: The % column shows the percentage of members that HSC 1892 shares with each listed object.

Visualization

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