HSC 2085

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0.38 UTI
0.29
CN
1.0
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 8.2 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2085 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Close Moderate extinction Near-solar metallicity Very young

Cavallo et al. (2024)
Silver sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 124.296 -42.203 1.209 -3.964 4.007 32.127
Cavallo et al. 2024 124.249 -42.238 1.202 – – –
Hunt & Reffert 2023 124.3 -42.24 1.199 -3.939 3.972 32.027

💡 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
Cavallo et al. 2024 0.98 1.18 – 5 -0.100 – – –
Hunt & Reffert 2023 0.81 0.89 1.52 7 – – – –

Visualization

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