HSC 603

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0.29 UTI
0.4
CN
0.19
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 21.1 [arcmin]
  • CN 0.4 Poorly populated
  • Cdens 0.19 Very loose
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 603 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Close Low extinction Near-solar metallicity Intermediate age

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 – 298.975 41.615 0.943 0.516 -0.716 -3.833
Hu & Soubiran 2025 298.122 41.116 – – – –
Zhang et al. 2024 299.01 41.605 – – – –
Cavallo et al. 2024 298.122 41.116 0.954 – – –
Hunt & Reffert 2023 299.01 41.605 0.948 0.527 -0.62 -5.782

💡 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
Hu & Soubiran 2025 – – – – -0.160* – – –
Zhang et al. 2024 – – – – 0.026* – – –
Cavallo et al. 2024 0.97 0.72 – 617 -0.220 – – –
Hunt & Reffert 2023 1.00 0.30 1.03 207 – – – –

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

Visualization

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