HSC 1627

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0.24 UTI
0.0
CN
0.1
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 7.4 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.1 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1627 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, well above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It was recently reported in the literature.
Relatively close Low extinction Near-solar metallicity Old

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 – 112.017 12.066 0.335 -0.567 -0.623 59.557
Hu & Soubiran 2025 112.028 12.131 – – – –
Zhang et al. 2024 112.022 12.025 – – – –
Hunt & Reffert 2024 112.022 12.025 0.321 -0.529 -0.681 52.17
Cavallo et al. 2024 112.028 12.131 0.329 – – –
Hunt & Reffert 2023 112.022 12.025 0.321 -0.529 -0.681 52.17

💡 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 – – – – -0.190* – – –
Zhang et al. 2024 – – – – -0.225* – – –
Hunt & Reffert 2024 – – – – – 59* – –
Cavallo et al. 2024 2.77 0.47 – 2818 -0.310 – – –
Hunt & Reffert 2023 3.08 0.75 1.00 986 – – – –

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

Visualization

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