HSC 1860

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0.41 UTI
0.51
CN
0.3
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 2.7 [arcmin]
  • CN 0.51 Moderately populated
  • Cdens 0.3 Loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1860 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a large* distance, well below the mid-plane, affected by low extinction. It is catalogued as a metal-poor, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It was recently reported in the literature.

(*): The parallax distance estimate (~7.53 kpc) differs significantly from the median photometric distance (~5.30 kpc).

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

Very distant Low extinction Metal-poor 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 – 104.278 -23.565 0.133 -0.42 2.0 72.602
Hu & Soubiran 2025 104.287 -23.576 – – – –
Hunt & Reffert 2024 104.284 -23.573 0.128 -0.42 1.972 72.601
Cavallo et al. 2024 104.287 -23.576 0.13 – – –
Hunt & Reffert 2023 104.284 -23.573 0.128 -0.42 1.972 72.601

💡 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 – – – – -0.390* – – –
Hunt & Reffert 2024 – – – – – 254* – –
Cavallo et al. 2024 3.60 0.62 – 1000 -0.860 – – –
Hunt & Reffert 2023 7.01 0.41 1.63 690 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 2968 94.2 104.28 -23.57 0.12 -0.42 2.0 72.6 0.02

💡 Note: The % column shows the percentage of members that HSC 1860 shares with each listed object.

Visualization

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