HSC 2140

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0.40 UTI
0.0
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.8
Cdup
Radius (P>50% members) 0.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.8 Very likely unique

Overview

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HSC 2140 is a sparse, very dense object of very high 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 age parameter (see Parameters). It was recently reported in the literature.

Note: This is very likely a unique object, which shares a small percentage of members with at least one previously 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 – 131.176 -46.151 0.214 -3.306 3.934 –
Hu & Soubiran 2025 131.181 -46.141 – – – –
Hunt & Reffert 2024 131.18 -46.151 0.212 -3.293 3.926 –
Cavallo et al. 2024 131.181 -46.141 0.209 – – –
Hunt & Reffert 2023 131.18 -46.151 0.212 -3.293 3.926 –

💡 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 – – – – – 172* – –
Cavallo et al. 2024 3.08 1.52 – 562 -0.230 – – –
Hunt & Reffert 2023 4.32 2.01 0.61 114 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3263 92.0 131.18 -46.15 0.2 -3.3 3.94 – 0.08
Bochum 7 20.0 131.2 -45.99 0.19 -3.39 3.87 – 0.27

💡 Note: The % column shows the percentage of members that HSC 2140 shares with each listed object.

Visualization

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