HSC 2106

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0.22 UTI
0.5
CN
0.27
Cdens
0.75
CC3
0.0
Clit
0.72
Cdup
Radius (P>50% members) 25.4 [arcmin]
  • CN 0.5 Moderately populated
  • Cdens 0.27 Loose
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.72 Likely unique

Overview

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HSC 2106 is a moderately populated, loose object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a metal-rich, 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.

Close Low extinction Metal-rich Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 130.974 -41.968 1.207 -8.233 5.784 26.262
Cavallo et al. 2024 130.811 -41.631 1.209 – – –
Hunt & Reffert 2023 130.894 -41.853 1.209 -8.206 5.787 28.306

💡 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
Cavallo et al. 2024 0.87 0.23 – 135 0.520 – – –
Hunt & Reffert 2023 0.78 0.20 0.85 313 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1194 28.0 130.38 -41.31 1.22 -8.08 5.77 28.36 0.2

💡 Note: The % column shows the percentage of members that HSC 2106 shares with each listed object.

Visualization

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