HSC 2239

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0.20 UTI
0.41
CN
0.09
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Core radius and density 1.8 [pc], 0.5 [pc-2]
  • CN 0.41 Poorly populated
  • Cdens 0.09 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
HSC 2239 is a poorly populated, very loose object of intermediate 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, young 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.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Palma et al. (2025)
Part of multiple system G147, along with HSC_2266, Theia_453 and Theia_1170.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as moving group. CMD class: 0.99 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.99 (50th percentile).

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 144.296 -53.147 1.52 -9.264 5.503 5.411
Cavallo et al. 2024 144.273 -53.215 1.516 – – –
Hunt & Reffert 2023 143.795 -53.151 1.516 -9.227 5.473 6.858

💡 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– 0.65 0.43 0.45 87 -0.280 – – –
Cavallo et al. 2024 0.67 0.69 – 62 -0.280 – – –
Hunt & Reffert 2023 0.63 0.17 0.45 112 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 3709 100.0 144.41 -53.24 1.52 -9.27 5.48 5.19 0.07

💡 Note: The % column shows the percentage of members that HSC 2239 shares with each listed object.

Visualization

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