HSC 2112

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0.38 UTI
0.29
CN
1.0
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 0.9 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2112 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, 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 High extinction Massive Metal-rich 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 – 133.948 -40.996 0.175 -2.789 2.62 76.457
Hunt & Reffert 2024 133.947 -40.996 0.16 -2.787 2.631 81.013
Cavallo et al. 2024 133.939 -40.995 0.16 – – –
Hunt & Reffert 2023 133.947 -40.996 0.16 -2.787 2.631 81.013

💡 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 – – – – – 1238* – –
Cavallo et al. 2024 3.98 3.17 – 389 0.570 – – –
Hunt & Reffert 2023 5.67 3.96 2.05 104 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3145 100.0 133.95 -41.0 0.17 -2.77 2.62 71.87 0.22

💡 Note: The % column shows the percentage of members that HSC 2112 shares with each listed object.

Visualization

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