HSC 2239

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0.27 UTI
0.41
CN
0.44
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 22.5 [arcmin]
  • CN 0.41 Poorly populated
  • Cdens 0.44 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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HSC 2239 is a poorly populated, 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.

Close Low extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 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] Bfr BSS
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 0.1

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

Visualization

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