HSC 1408

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0.27 UTI
0.0
CN
0.08
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 0.4 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.08 Very loose
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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HSC 1408 is a sparse, very loose object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It was recently reported in the literature.

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

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 99999– 82.002 27.792 0.17 0.676 -1.129 –
Hu & Soubiran 2025 81.985 27.8 – – – –
Hunt & Reffert 2024 81.99 27.83 0.181 0.668 -1.126 –
Cavallo et al. 2024 81.985 27.8 0.177 – – –
Hunt & Reffert 2023 81.99 27.83 0.181 0.668 -1.126 –

💡 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] Bfrac BSS
UCC 99999– 5.52 1.815 0.77 1287 -0.205 509 – –
Hu & Soubiran 2025 – – – – -0.260(5) – – –
Hunt & Reffert 2024 – – – – – 509(1) – –
Cavallo et al. 2024 6.31 1.98 – 832 -0.150 – – –
Hunt & Reffert 2023 4.73 1.65 0.77 1742 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3674 100.0 82.0 27.8 0.21 0.68 -1.11 – 0.14

💡 Note: The % column shows the percentage of members that HSC 1408 shares with each listed object.

Visualization

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