HSC 2651

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0.37 UTI
0.0
CN
0.6
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.6 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 2651 is a sparse, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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 – 217.478 -61.137 0.472 -3.801 -3.076 –
Hu & Soubiran 2025 217.519 -61.14 – – – –
Hunt & Reffert 2024 217.463 -61.14 0.474 -3.82 -3.079 –
Cavallo et al. 2024 217.52 -61.14 0.474 – – –
Hunt & Reffert 2023 217.463 -61.14 0.474 -3.82 -3.079 –

💡 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 – – – – -0.120* – – –
Hunt & Reffert 2024 – – – – – 133* – –
Cavallo et al. 2024 1.70 1.81 – 676 0.180 – – –
Hunt & Reffert 2023 2.02 1.96 0.41 124 – – – –

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

Visualization

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