HSC 2082

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0.47 UTI
0.6
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 6.7 [N/pc2]
  • CN 0.6 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2082 is a moderately populated, very dense 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 near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Palma et al. (2025)
Part of multiple system G137, along with Theia_773, Theia_274, Theia_986, HSC_2085 and Theia_2103.

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 99999– 124.543 -41.825 1.231 -4.755 10.283 26.569
Hunt & Reffert 2024 124.547 -41.823 1.213 -4.745 10.236 27.469
Cavallo et al. 2024 124.497 -41.853 1.225 – – –
Hunt & Reffert 2023 124.547 -41.823 1.213 -4.745 10.236 27.469

💡 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] Bfrac BSS
UCC 99999– 0.795 0.705 1.43 340 0.270 134 – –
Hunt & Reffert 2024 – – – – – 134(1) – –
Cavallo et al. 2024 0.81 0.69 – 309 0.270 – – –
Hunt & Reffert 2023 0.78 0.72 1.43 372 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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