HSC 502

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0.02 UTI
0.0
CN
0.01
Cdens
0.38
CC3
0.0
Clit
0.28
Cdup
Stellar density (N50/rad) 0.1 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.01 Very loose
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.28 Possibly duplicate

Overview

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HSC 502 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very large distance, well above the mid-plane. It is catalogued as a massive cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 294.798 26.254 0.05 -2.254 -4.373 –
Hunt & Reffert 2024 294.799 26.263 0.054 -2.27 -4.372 -79.359

💡 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– – – – – – 4065 – –
Hunt & Reffert 2024 – – – – – 4065(1) – –

(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 4386 72.0 294.77 26.21 0.06 -2.26 -4.39 – 0.08

💡 Note: The % column shows the percentage of members that HSC 502 shares with each listed object.

Visualization

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