HSC 679

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0.41 UTI
0.33
CN
0.97
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.33 Poorly populated
  • Cdens 0.97 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 679 is a poorly 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 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.

Relatively close High 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 – 311.206 47.602 0.312 -3.923 -4.233 -20.495
Hunt & Reffert 2024 311.203 47.596 0.312 -3.913 -4.241 -20.629
Cavallo et al. 2024 311.211 47.606 0.312 – – –
Hunt & Reffert 2023 311.203 47.596 0.312 -3.913 -4.241 -20.629

💡 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 – – – – – 533* – –
Cavallo et al. 2024 2.92 3.92 – 174 0.100 – – –
Hunt & Reffert 2023 2.77 4.17 2.42 106 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3563 100.0 311.21 47.6 0.3 -3.92 -4.24 -20.49 0.1

💡 Note: The % column shows the percentage of members that HSC 679 shares with each listed object.

Visualization

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