HSC 868

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0.32 UTI
0.63
CN
0.96
Cdens
0.75
CC3
0.0
Clit
0.68
Cdup
Radius (P>50% members) 3.7 [arcmin]
  • CN 0.63 Moderately populated
  • Cdens 0.96 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.68 Likely unique

Overview

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HSC 868 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, 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.

Relatively close High extinction Massive Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 343.424 62.813 0.27 -1.983 -1.008 -56.862
Hunt & Reffert 2024 343.461 62.819 0.274 -2.003 -1.003 -56.887
Cavallo et al. 2024 343.446 62.82 0.275 – – –
Hunt & Reffert 2023 343.461 62.819 0.274 -2.003 -1.003 -56.887

💡 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 – – – – – 1062* – –
Cavallo et al. 2024 2.39 3.37 – 372 -0.260 – – –
Hunt & Reffert 2023 3.33 3.43 2.17 74 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3365 100.0 343.44 62.81 0.27 -1.99 -1.02 -56.86 0.21
FoF 1822 31.6 343.41 62.82 0.26 -2.11 -1.01 -101.64 0.28

💡 Note: The % column shows the percentage of members that HSC 868 shares with each listed object.

Visualization

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