HSC 2612

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0.13 UTI
0.52
CN
0.61
Cdens
0.75
CC3
0.0
Clit
0.36
Cdup
Stellar density (N50/rad) 3.0 [N/pc2]
  • CN 0.52 Moderately populated
  • Cdens 0.61 Moderately dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.36 Possibly duplicate

Overview

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HSC 2612 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, young cluster (see Parameters). It was recently reported in the literature.

âš ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.

Palma et al. (2025)
Part of multiple system G161, along with Theia_2651, CWNU_2631 and OC_0600.

Cavallo et al. (2024)
Bronze 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– 207.435 -62.877 0.3 -6.393 -1.981 7.208
Hunt & Reffert 2024 207.406 -62.872 0.301 -6.474 -1.963 -20.403
Cavallo et al. 2024 207.532 -62.864 0.298 – – –
Hunt & Reffert 2023 207.406 -62.872 0.301 -6.474 -1.963 -20.403

💡 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– 3.35 4.17 3.03 39 0.630 1876 – –
Hunt & Reffert 2024 – – – – – 1876(1) – –
Cavallo et al. 2024 3.61 4.10 – 49 0.630 – – –
Hunt & Reffert 2023 3.09 4.24 3.03 29 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
G3CC 13 64.2 207.42 -62.87 0.31 -6.33 -2.02 -11.19 0.52
CWNU 3462 58.5 207.42 -62.87 0.31 -6.34 -2.02 -24.51 0.06
CWNU 3597 20.8 207.69 -62.86 0.3 -6.67 -1.88 -61.79 0.43

💡 Note: The % column shows the percentage of members that HSC 2612 shares with each listed object.

Visualization

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