HSC 1865

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0.01 UTI
0.8
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.01
Cdup
Radius (P>50% members) 15.6 [arcmin]
  • CN 0.8 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 0.01 Very likely duplicate

Overview

â„šī¸
HSC 1865 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Close Low extinction Near-solar metallicity Very young

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 – 103.6 -24.216 1.121 -2.812 3.519 37.369
Wei et al. 2025 103.637 -24.216 1.146 -2.809 3.522 –
Hunt & Reffert 2024 103.663 -24.234 1.122 -2.819 3.505 35.285
Cavallo et al. 2024 103.558 -24.247 1.124 – – –
Hunt & Reffert 2023 103.663 -24.234 1.122 -2.819 3.505 35.285

💡 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
Wei et al. 2025 0.74 0.77 – 3 -0.250 825 0.51 –
Hunt & Reffert 2024 – – – – – 325* – –
Cavallo et al. 2024 0.87 0.53 – 5 -0.360 – – –
Hunt & Reffert 2023 0.86 0.16 0.75 8 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2270 99.2 103.55 -24.25 1.12 -2.81 3.52 37.37 0.56

💡 Note: The % column shows the percentage of members that HSC 1865 shares with each listed object.

Visualization

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