HSC 529

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0.20 UTI
0.0
CN
1.0
Cdens
0.62
CC3
0.0
Clit
0.6
Cdup
Radius (P>50% members) 1.7 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.6 Likely unique

Overview

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HSC 529 is a sparse, very 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.

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.

Distant Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Silver sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 298.67 29.795 0.233 -2.457 -4.845 –
Hunt & Reffert 2024 298.668 29.8 0.23 -2.476 -4.838 –
Cavallo et al. 2024 298.659 29.801 0.231 – – –
Hunt & Reffert 2023 298.668 29.8 0.23 -2.476 -4.838 –

💡 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
Hunt & Reffert 2024 – – – – – 271* – –
Cavallo et al. 2024 4.43 2.14 – 234 -0.330 – – –
Hunt & Reffert 2023 4.22 2.72 1.01 7 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4799 84.0 298.67 29.8 0.23 -2.45 -4.85 – 0.04
FoF 1728 40.0 298.73 29.91 0.23 -2.41 -4.87 – 0.11

💡 Note: The % column shows the percentage of members that HSC 529 shares with each listed object.

Visualization

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