HSC 280

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0.01 UTI
0.0
CN
0.02
Cdens
0.12
CC3
0.0
Clit
0.48
Cdup
Stellar density (N50/rad) 0.1 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 0.48 Possibly duplicate

Overview

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HSC 280 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large distance, above the mid-plane. It is catalogued as an extremely 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– 276.845 -2.409 0.156 -2.158 -4.747 58.426
Hunt & Reffert 2024 276.842 -2.394 0.184 -2.049 -4.666 40.613

💡 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– – – – – – 38380 – –
Hunt & Reffert 2024 – – – – – 38380(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 4792 52.0 276.85 -2.41 0.14 -2.16 -4.95 – 0.08

💡 Note: The % column shows the percentage of members that HSC 280 shares with each listed object.

Visualization

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