HSC 2065

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0.00 UTI
0.0
CN
0.03
Cdens
0.75
CC3
0.0
Clit
0.0
Cdup
Stellar density (N50/rad) 0.1 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.03 Very loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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HSC 2065 is a sparse, very loose object of high C3 quality. Its parallax locates it at a very large distance, well below the mid-plane. It is catalogued as a cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large 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– 121.786 -41.305 0.074 -1.364 2.184 126.61
Hunt & Reffert 2024 121.792 -41.295 0.063 -1.361 2.207 126.36

💡 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– – – – – – 623 – –
Hunt & Reffert 2024 – – – – – 623(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 3876 100.0 121.78 -41.31 0.07 -1.36 2.19 126.61 0.24

💡 Note: The % column shows the percentage of members that HSC 2065 shares with each listed object.

Visualization

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