HSC 103

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0.12 UTI
0.25
CN
0.21
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 166.9 [arcmin]
  • CN 0.25 Poorly populated
  • Cdens 0.21 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 103 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a metal-rich, young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Very close Low extinction Metal-rich Young

Cavallo et al. (2024)
Bronze 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 – 269.526 -21.999 9.904 -6.593 -39.598 -10.083
Cavallo et al. 2024 271.179 -22.524 9.96 – – –
Hunt & Reffert 2023 269.21 -22.05 9.96 -6.15 -39.558 9.598

💡 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 0.09 1.15 – 170 0.510 – – –
Hunt & Reffert 2023 0.10 0.28 0.63 4 – – – –

Visualization

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