HSC 2339

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0.14 UTI
0.0
CN
1.0
Cdens
0.5
CC3
0.0
Clit
0.48
Cdup
Stellar density (N50/rad) 10.2 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.48 Possibly duplicate

Overview

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HSC 2339 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very 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)
Classified as optical pair P463, along with Theia_3227.

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– 156.471 -58.578 0.266 -5.383 2.989 –
Hunt & Reffert 2024 156.456 -58.587 0.261 -5.368 2.994 –
Cavallo et al. 2024 156.456 -58.586 0.261 – – –
Hunt & Reffert 2023 156.456 -58.587 0.261 -5.368 2.994 –

💡 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– 4.32 2.965 1.97 13 -0.400 861 – –
Hunt & Reffert 2024 – – – – – 861(1) – –
Cavallo et al. 2024 4.76 3.13 – 8 -0.400 – – –
Hunt & Reffert 2023 3.88 2.80 1.97 18 – – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0542 52.0 156.6 -58.55 0.27 -5.39 3.04 – 0.1

💡 Note: The % column shows the percentage of members that HSC 2339 shares with each listed object.

Visualization

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