HSC 1977

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0.31 UTI
0.25
CN
0.8
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 52.7 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.8 Dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 1977 is a poorly populated, dense object of intermediate C3 quality. Its parallax locates it at a very close distance, near 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.
Very 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 – 98.85 -36.732 6.119 -10.362 21.25 28.55
Cavallo et al. 2024 98.325 -36.505 6.124 – – –
Hunt & Reffert 2023 98.821 -36.716 6.125 -10.022 21.195 29.126

💡 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 0.17 0.32 – 40 0.330 – – –
Hunt & Reffert 2023 0.16 0.01 0.48 24 – – – –

Visualization

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