HSC 672

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0.34 UTI
0.0
CN
0.57
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.3 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.57 Moderately dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 672 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.
Relatively close Moderate 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 – 307.383 49.05 0.45 -2.396 -5.396 -46.894
Hu & Soubiran 2025 307.386 49.035 – – – –
Hunt & Reffert 2024 307.375 49.052 0.455 -2.4 -5.372 -42.634
Cavallo et al. 2024 307.386 49.035 0.458 – – –
Hunt & Reffert 2023 307.375 49.052 0.455 -2.4 -5.372 -42.634

💡 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 – – – – -0.060* – – –
Hunt & Reffert 2024 – – – – – 136* – –
Cavallo et al. 2024 1.94 2.42 – 603 0.000 – – –
Hunt & Reffert 2023 2.14 1.92 1.73 693 – – – –

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

Visualization

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