HSC 406

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0.04 UTI
0.0
CN
0.09
Cdens
0.25
CC3
0.0
Clit
0.56
Cdup
Stellar density (N50/rad) 0.5 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.09 Very loose
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.56 Likely unique

Overview

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HSC 406 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P51, along with King_25.

Cavallo et al. (2024)
Bronze 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– 290.252 13.604 0.317 -1.572 -4.535 24.117
Hunt & Reffert 2024 290.289 13.588 0.318 -1.587 -4.503 24.095
Cavallo et al. 2024 290.263 13.591 0.321 – – –
Hunt & Reffert 2023 290.289 13.588 0.318 -1.587 -4.503 24.095

💡 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– 3.27 4.81 2.69 13 -0.090 967 – –
Hunt & Reffert 2024 – – – – – 967(1) – –
Cavallo et al. 2024 3.75 4.67 – 12 -0.090 – – –
Hunt & Reffert 2023 2.79 4.95 2.69 14 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0126 44.0 290.27 13.7 0.32 -1.61 -4.53 18.9 0.3

💡 Note: The % column shows the percentage of members that HSC 406 shares with each listed object.

Visualization

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