HSC 1735

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0.32 UTI
0.0
CN
0.71
Cdens
0.38
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.71 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1735 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a moderate 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.
Relatively close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 112.63 -2.608 0.466 -1.395 -0.323 52.807
Hu & Soubiran 2025 112.635 -2.602 – – – –
Hunt & Reffert 2024 112.631 -2.609 0.47 -1.389 -0.332 –
Cavallo et al. 2024 112.634 -2.601 0.47 – – –
Hunt & Reffert 2023 112.631 -2.609 0.47 -1.389 -0.332 –

💡 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 – – – – -0.220* – – –
Hunt & Reffert 2024 – – – – – 81* – –
Cavallo et al. 2024 2.11 0.21 – 1259 -0.010 – – –
Hunt & Reffert 2023 1.89 0.11 0.36 659 – – – –

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

Visualization

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