HSC 2012

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0.26 UTI
0.3
CN
0.52
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 19.6 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.52 Moderately dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2012 is a poorly populated, moderately dense object of intermediate 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, young cluster (see Parameters). It was recently reported in the literature.
Close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold 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 – 110.514 -37.447 1.673 -7.803 7.716 31.112
Cavallo et al. 2024 110.367 -37.331 1.636 – – –
Hunt & Reffert 2023 110.468 -37.453 1.639 -7.773 7.636 22.738

💡 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 0.68 0.64 – 13 0.000 – – –
Hunt & Reffert 2023 0.59 0.21 0.73 33 – – – –

Visualization

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