HSC 682

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0.35 UTI
0.49
CN
1.0
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.3 [arcmin]
  • CN 0.49 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.25 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 682 is a poorly populated, very dense object of low 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 object shares a large percentage of members with a later 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 – 313.108 46.925 0.255 -3.268 -4.048 -43.329
Hunt & Reffert 2024 313.115 46.93 0.246 -3.257 -4.069 -43.487
Cavallo et al. 2024 313.111 46.924 0.249 – – –
Hunt & Reffert 2023 313.115 46.93 0.246 -3.257 -4.069 -43.487

💡 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 – – – – – 710* – –
Cavallo et al. 2024 3.31 2.18 – 263 0.000 – – –
Hunt & Reffert 2023 3.49 2.28 2.88 117 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3201 100.0 313.1 46.92 0.25 -3.25 -4.04 -50.7 0.15

💡 Note: The % column shows the percentage of members that HSC 682 shares with each listed object.

Visualization

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